The galaxy presents as a relatively smooth, elliptical or lenticular object with an overall round morphology. There's no apparent spiral arm structure, but instead a generally uniform distribution of light. Color gradients suggest some internal structure, with a slightly bluer core fading into a redder halo, indicative of possible radial variations in stellar populations or dust content. There is no indication of ongoing major merger activity. There may be minor asymmetries or perturbations hinting at a potential minor interaction, although these could also be artifacts. The estimated size suggests a substantial galaxy.
