This galaxy presents as a moderately bright elliptical, appearing largely featureless and smooth in overall structure. The light distribution seems concentrated towards the center, indicating a well-defined nucleus, with a gradual decrease in luminosity moving outwards. The galaxy is nearly circular, showing little ellipticity. Color gradients are subtle, though there may be a slight redder hue towards the central regions, suggestive of an older stellar population. There is no visible evidence of spiral arms or a prominent disk component, based on the general composition of the galaxy. No signs of any major ongoing merger events are evident, based on a lack of significant tidal tails or disrupted morphology. There appear to be some minor visual irregular components.
