The galaxy presents a largely smooth morphology, appearing elliptical in shape. The light profile indicates a concentrated central bulge, possibly harboring a supermassive black hole. This central region exhibits a yellowish hue, suggestive of an older stellar population. Moving outwards from the core, there is a gradual decrease in luminosity. There appears to be a faint disk surrounding the main region, with a blue color. This would possibly indicate ongoing star formation. Overall, the galaxy appears to be an intermediate mass system. There are no indications of any major mergers happening, but there are possible minor disturbances visible on the right side.
