The galaxy presents an elliptical, disk-like structure with a noticeable central bulge. The bulge appears relatively bright and concentrated. The disk, extending outward from the central bulge, exhibits a relatively smooth texture. The outer regions of the galaxy show some subtle features, hinting at a possible spiral arm structure. The galaxy's orientation is tilted with respect to our line of sight. The overall color profile suggests a relatively evolved stellar population within the bulge, while the disk exhibits slightly bluer hues, possibly indicating regions of ongoing star formation. There is no strong evidence of any major ongoing merger activity or significant tidal disturbances based on the galaxy's morphology. There is a suggestion of the presence of a weak bar structure near the center of the galaxy.
