The galaxy presents as a somewhat lenticular or possibly edge-on spiral galaxy. The overall shape is elongated, with an axis ratio suggesting a moderate inclination relative to our line of sight. A central bulge is evident, appearing relatively smooth and centrally concentrated. Fainter, diffuse disk components extend outwards from the bulge.

The color gradient suggests a redder core region that might denote an older stellar population with diminished star formation, whereas bluer tinges within the disk may represent ongoing or more recent star formation. However, significant dust obscuration may be present, affecting observed colors and potentially masking star-forming regions. There are hints of slight asymmetry or possible tidal features, suggesting a potential gravitational interaction or minor merger event, but these features are not strongly defined.
