The galaxy appears as a relatively compact object. Its light profile suggests a spheroidal morphology with a dominant central bulge, and a smoother overall texture, with minimal evidence of spiral arms or other disk-like features. Color gradients indicate a concentration of older stellar populations in the central region, characterized by reddish hues. Fainter, bluer regions, possibly indicative of more recent star formation, can be observed. There is a slight asymmetry visible in the outer regions, which might suggest a minor interaction. The object appears generally isolated, without prominent signs of recent or ongoing major mergers or tidal disruptions.
