The galaxy presents as a concentrated, elliptical-like system. It exhibits a smooth, relatively featureless morphology, without any discernible spiral arms or distinct disk-like structure. The central bulge appears dominant and relatively bright, with a gradual decrease in luminosity outwards. The galaxy's color gradient transitions from a yellowish core to a slightly bluer halo, suggesting a differential stellar population distribution, with older, redder stars concentrated in the center and younger, bluer stars in the outer regions. The overall shape is somewhat elongated but not highly so, appearing more oval than cigar-shaped. There is no evidence of significant tidal disturbances or ongoing major merging activity, though the possibility of minor interactions cannot be entirely ruled out given the image's resolution.
