The galaxy presents as a relatively smooth, centrally concentrated object, likely an elliptical or lenticular galaxy. Its shape appears largely rounded. There is little evidence of spiral arm structure or significant dust lanes. The central region exhibits a brighter core, suggesting a possible active galactic nucleus or a dense concentration of stars. The galaxy's color indices suggest a population of older stars, with a relatively low rate of ongoing star formation. There is a low probability of any ongoing major merger events, with some possible minor tidal disturbances present. Overall, the galaxy appears as a fairly evolved system.
