The galaxy presents a largely smooth, elliptical morphology, with minimal apparent substructure. Its overall shape is generally rounded, appearing somewhat oblate rather than highly elongated. The light distribution shows a centrally concentrated luminosity profile, with the highest intensity emission originating from the core region. A gradual decrease in surface brightness extends outwards from the nucleus, with no distinct spiral arms or prominent dust lanes visible in the available imagery.

The color of the galaxy appears overall yellowish, suggestive of a stellar population dominated by older, more evolved stars. The lack of strong blue emission suggests a relatively low rate of on-going star formation. There is no readily apparent evidence of any major tidal disturbances or interactions with other galaxies.
