The galaxy presents a generally smooth and elliptical morphology. The light profile appears concentrated towards the center, with a gradual decrease in intensity towards the outer regions. There is an apparent lack of distinct spiral arm structures or prominent dust lanes. The galaxy exhibits a yellowish-white hue, suggestive of an older stellar population. There's no obvious evidence of ongoing major mergers or tidal disturbances. The isophotes appear to be moderately elliptical, indicating a shape somewhere between a perfect circle and a cigar-like ellipse. The galaxy seems to be a relatively isolated system.