The galaxy presents a generally smooth, elliptical morphology. The light profile appears centrally concentrated, exhibiting a brighter, more intensely colored core that fades gradually toward the outer edges. The color distribution is not uniform; the central region displays a yellowish-orange hue suggesting an older stellar population, while the periphery appears slightly bluer, indicating the presence of some younger, hotter stars or ongoing star formation at a lower rate relative to the core. There is a subtle suggestion of a very faint, diffuse disk or spiral structure, but the overall impression is that of a spheroid-dominated system. The galaxy's overall structure appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions. There may be a very minor, faint distortion in the morphology, suggesting a possible minor interaction. It is neither perfectly round nor cigar-shaped.
