The galaxy presents as an elliptical morphology, exhibiting a smooth, largely featureless light distribution. Its overall color is indicative of an older stellar population, trending towards the redder end of the spectrum. The galaxy's structure appears undisturbed, with no obvious signs of tidal interactions or ongoing major mergers, though a subtle asymmetry may suggest a minor interaction or past disturbance. The central region of the galaxy appears slightly more concentrated, with a gradual decrease in luminosity towards the outer edges. The shape is nearly round with a tendency towards a very slight elongation.
