The galaxy presents as an elliptical or lenticular structure. Its overall shape is smooth, lacking prominent spiral arms or irregular features. The light distribution shows a central bulge that gradually fades outwards. The core exhibits a yellowish-white hue, potentially indicating an older stellar population. The outer regions show a subtle shift towards reddish tones suggesting the presence of some dust or a population of older, redder stars. There is no obvious evidence of ongoing major mergers or tidal disturbances. The galaxy's shape appears to be primarily spheroidal, with a slight elongation visible.
