The galaxy presents a largely smooth morphology, exhibiting minimal evidence of distinct spiral arms or a pronounced disk structure. The light distribution is concentrated towards the center, suggesting a prominent galactic bulge. The overall shape appears nearly circular. There is a subtle color gradient visible, with a yellow-orange hue dominating the central region, potentially indicative of an older stellar population. The outer regions are slightly bluer in comparison, which could be due to younger stars, but the feature is very subtle. There is no clear indication of active star formation based on the available image data, and no obvious signs of an ongoing merger or tidal disturbances. Overall, the galaxy is consistent with an elliptical galaxy at a redshift of roughly 0.1.
