The galaxy presents as a somewhat elongated, disk-like structure. It appears to be dominated by an elliptical, yellowish bulge, indicative of an older stellar population. Fainter, bluer regions can be discerned along the outer edges of the disk, suggesting the presence of younger, hotter stars, and thus possible ongoing star formation, albeit at a modest rate. The overall structure lacks any clear spiral arm features and exhibits a relatively smooth appearance. There is a slight hint of asymmetry in the distribution of the bluer regions, which could potentially indicate a minor gravitational interaction or disturbance, but more data would be needed to be confident of such. The overall form suggests a galaxy somewhere between a pure elliptical and a more structured spiral, possibly a lenticular type galaxy.
