The galaxy presents as an elliptical morphology, exhibiting a predominantly smooth structure. The central region displays a concentrated luminosity, transitioning to a more diffuse halo. The overall color gradient is relatively subtle, showing a slightly reddish hue in the core possibly indicating an older stellar population, fading into a blue tinge further out. The elongated shape of the galaxy suggests a moderate degree of ellipticity, but no apparent spiral arm structure or prominent dust lanes are observed in this image. There is no indication of a recent or ongoing major merger event, although a minor interaction may be plausible, based on some slight asymmetries in the outer regions. The galaxy's overall appearance aligns with that of a relatively quiescent system with a modest star formation rate.
