The galaxy presents as a relatively smooth, elliptical structure. It is characterized by a concentrated, bright central region that appears spheroidal. The light distribution shows a gradient decreasing from the center outwards. The core is predominantly yellowish-orange, indicating a population of older stars. There's a subtle indication of bluer light in the surrounding regions, suggesting some ongoing or recent star formation, albeit at a low level. The overall morphology lacks any obvious spiral arms or significant dust lanes, further supporting its classification as an elliptical galaxy. There is no clear evidence of any major tidal interactions or merging events. Based on the round shape and its smooth features, this galaxy appears to be in a relatively relaxed state.
