The galaxy presents as a moderately bright, well-defined elliptical structure. Its overall form is notably smooth with no apparent spiral arm features or prominent dust lanes. The galaxy appears roughly circular in shape. The light distribution suggests a centrally concentrated bulge, gradually fading outwards towards the edges. There is a slight colour gradient observable, with the central region appearing somewhat redder compared to the outer regions, which exhibit a bluer hue. This suggests the presence of a relatively older stellar population in the core, and potentially ongoing star formation in the outer regions, although this is not immediately apparent. There is no visual evidence of any major mergers or tidal disturbances, indicating that this galaxy is likely to be relatively isolated and undisturbed.
