The galaxy presents as an elliptical morphology, with a smooth, diffuse light distribution. The central region exhibits a brighter, more concentrated luminosity, suggesting a possible galactic bulge. The overall color is slightly yellow-red, which could be indicative of an older stellar population and reduced ongoing star formation. A slight elongation is observed with a hint of a disc structure but is not well-defined. There are no obvious signs of a major merger, although a subtle asymmetry indicates the possibility of minor interactions or internal disturbances. The lack of distinct spiral arms, dust lanes, or bright, blue regions points away from a actively star-forming disk galaxy.