The galaxy presents as a somewhat smooth, elliptical-like structure. It has a concentrated central bulge with a yellowish hue, possibly indicative of an older stellar population. Diffuse arms or extended features emerge from this central region. These extensions exhibit a bluer tint, suggesting ongoing or recent star formation. There is a possible minor disruption, or an indication of tidal interaction on one end of the galaxy. The overall morphology suggests it is a galaxy in a transitional phase, potentially evolving from a more disk-like system to a more spheroidal structure.
