The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a round morphology, with a noticeable radial gradient in luminosity, brightest at the core and gradually fading outwards. The color profile suggests a population of older stars, indicated by the redder hue towards the central bulge. There is little evidence of spiral arm structure or significant dust lanes. Overall, the galaxy appears to be a quiescent, early-type system, potentially an elliptical galaxy. Minimal signs of recent or ongoing star formation are discernible from the image. There appears to be no major disturbances or signs of merging activity.
