The galaxy presents as a somewhat elongated elliptical structure. Its light profile appears concentrated towards the center, exhibiting a smooth, centrally-peaked morphology, with a gradual decrease in luminosity towards the outer edges. No distinct spiral arm structures or bar features are discernible. Color gradients are subtle, showing a tendency towards redder hues in the core region. This color is consistent with an older stellar population dominating the nuclear region, while the outer regions show a slightly bluer hue. The galaxy appears relatively undisturbed, with no obvious signs of major mergers or tidal interactions with neighboring galaxies. However, there may be minor disturbances or asymmetries in the outer envelope, hinting at the possibility of past minor mergers or accretion events.
