The galaxy presents a generally smooth, elliptical morphology. Its central region exhibits a concentrated, bright core, which gradually diffuses outward into a more extended halo. The overall color profile suggests an older stellar population, with a noticeable lack of prominent blue regions indicative of recent star formation. The galaxy appears slightly elongated, deviating from a perfectly circular shape, hinting at a possible cigar shape. There is no obvious evidence of major mergers or tidal disturbances, although subtle irregularities in the outer regions cannot be ruled out without further investigation. The relative smoothness indicates a likely evolved system.
