The galaxy presents a distinct morphology. It appears relatively smooth and compact, exhibiting a general spheroidal shape with a slight elongation, deviating marginally from a perfectly circular form. A luminosity gradient is observed, with the central region showing a higher surface brightness that fades outwards. The light distribution suggests a centrally concentrated stellar population. The galaxy's color is predominantly red, but has a slight blue color, suggesting the presence of intermediate-age stellar populations and possible ongoing star formation. There is no evidence of a prominent disk component, spiral arms, or a bar structure based on this image. No significant tidal features or other signs of recent major mergers are visible; however, minor disturbances cannot be ruled out. Overall, the galaxy is consistent with being a massive elliptical or lenticular galaxy.