The galaxy appears as a single, relatively smooth, centrally concentrated object. Its overall morphology suggests an elliptical or lenticular type. The galaxy displays a somewhat uniform color profile, trending towards the redder end of the spectrum, implying a population of older stars and a lack of significant ongoing star formation. There are no discernible spiral arms or prominent dust lanes. The shape appears roughly circular, with minimal deviation from a perfect circle. There is no clear visual evidence of any major ongoing merger activity or significant tidal disturbances, though minor asymmetries cannot be entirely ruled out at this resolution. The galaxy's luminosity seems high.
