The galaxy presents as a smooth, elliptical morphology. It exhibits a concentrated, bright central bulge that fades gradually towards the outer edges. The shape is not perfectly circular, appearing somewhat elongated or cigar-shaped. The color gradient suggests an older stellar population, with a yellowish-orange hue dominating the central regions, potentially indicating a lack of significant ongoing star formation. There are no distinct spiral arms or prominent dust lanes visible. No evidence of any major merging or tidal disturbances are seen. The galaxy appears relatively isolated and undisturbed.
