The galaxy presents as a single, fairly smooth object with a concentrated central bulge. There's a general elliptical morphology, tending towards round, with no significant distortions or tidal features readily apparent. The color gradient shows a yellower core, suggesting an older stellar population concentrated in the center. The outer regions of the galaxy become slightly bluer, which could indicate the presence of younger, hotter stars in those areas, though this feature is subtle. Star formation appears limited based on the overall color. The galaxy lacks any prominent spiral arms or distinct disk structure. There is no clear evidence of ongoing major merger activity or significant interaction with other galaxies. Some minor disturbances cannot be ruled out.
