The galaxy appears as a luminous, centrally concentrated object, with a smooth light distribution, indicating an elliptical morphology. The galaxy is slightly elongated, exhibiting a low degree of ellipticity. It has a generally homogenous texture with some hints of substructure in the form of faint, diffuse extensions or asymmetries, potentially indicative of minor tidal interactions or recent accretion events.

The color profile suggests a population of older stars dominating the emission. The central region exhibits a slightly yellow-red hue. Fainter, bluish-white regions surround the core, possibly suggesting an area of weak star formation activity. Overall, the galaxy shows characteristics typically associated with galaxies exhibiting low specific star formation rates.
