The galaxy appears to be a lenticular or possibly an elliptical galaxy, displaying a largely smooth morphology. It exhibits an elongated, cigar-like shape in its overall structure. The central bulge is prominent and appears relatively bright, with the light appearing to become dimmer farther from the center. There is a faint disk component observed. There appears to be evidence of some minor disturbances present, but not enough to be considered a major merger event. The color profile of the galaxy seems to have a redder hue, which would be consistent with an older stellar population and low star formation rate. There is a lack of distinct spiral arm structure that I can discern.
