The galaxy presents as a relatively smooth, centrally concentrated object with a round morphology. Its color profile suggests an older stellar population, with a core exhibiting a yellowish-orange hue, indicative of evolved stars. A fainter, bluer halo surrounds the core, potentially indicating more recent, though still relatively low-level, star formation activity. The galaxy lacks any prominent spiral arm structures or bar features, suggesting that it is likely an elliptical or lenticular galaxy. There is a subtle asymmetry to the outer regions, with a slightly elongated extension to one side, possibly the result of a minor past merger event or tidal interaction with another galaxy. Overall, the galaxy appears to be a mature, relatively quiescent system with a modest level of recent star formation.
