The galaxy presents as a smooth, elliptical morphology with a high degree of central concentration. It exhibits a moderate ellipticity, appearing somewhat cigar-shaped, but mostly in between round and cigar shaped. There is no apparent disk structure or spiral arms, nor is there evidence of significant dust lanes or patches. The color profile suggests an older stellar population, with a general lack of blue light indicating low current star formation activity. There are no readily apparent signs of recent or ongoing merger activity, such as tidal tails or significant morphological distortions, although the presence of some minor disturbances cannot be ruled out completely at this resolution. The galaxy's light profile fades gradually from the bright central core, extending into a relatively featureless halo.
