The galaxy presents as a relatively smooth, elliptical object. The central region exhibits a high surface brightness, appearing yellowish-white, suggestive of an older stellar population. The galaxy exhibits a slight elongation, with the ratio of major to minor axis being approximately 5:4, indicating it is not perfectly spherical. Faint and diffuse extensions are observed extending from the main body, with hints of reddish color suggesting regions of ongoing or recent star formation. These features appear minimal, though, as the overall impression is that of a galaxy dominated by an older, more evolved stellar population and a smoothly distributed light profile. There is no obvious sign of a spiral structure or a significant dust lane. The galaxy appears relatively undisturbed, with no strong evidence of tidal tails or ongoing mergers with other galaxies.
