The galaxy presents as an elliptical-like system, though with subtle features suggesting it may not be a perfect ellipsoid. There is a central bulge exhibiting a bright, concentrated luminosity gradient. This region appears to be older stellar populations, indicated by its yellow-red hue. 

Extending outwards from the bulge, the galaxy exhibits a more diffuse and bluer component, possibly a faint, poorly defined disk. This area seems to show some level of recent star formation, with faint blue tinges and possibly a low specific star formation rate, suggested by the minimal blueness.

The overall structure suggests a system transitioning between a pure elliptical and a spiral, or a spiral that has undergone significant morphological transformation. There is a possible minor disturbance present at the lower edge of the galaxy. This could be the result of a past or ongoing minor merger event. The lack of strong tidal features suggests that any interaction is either minor or in its early stages. 

The galaxy appears relatively smooth overall, although the potential disturbance could be indicative of a more complex underlying structure.
