The galaxy presents a primarily smooth morphology, suggesting a classification leaning towards elliptical or lenticular. It exhibits a concentrated central bulge that appears yellowish-white, indicating a significant population of older stars. A faint, diffuse disk is suspected, but it is not well-defined. The overall color gradient transitions to a slightly bluer hue in the outer regions compared to the core, hinting at possible ongoing, albeit subdued, star formation in these areas. The galaxy's shape is generally rounded, though a subtle elongation might be present. There is a possibility of minor tidal disturbances or interactions with other galaxies, seen with a slight asymmetry in the disk region, but the overall structure does not suggest a major merger event. 
