The galaxy presents a generally smooth, elliptical morphology with a bright, concentrated central bulge. The light distribution appears relatively uniform, showing a gradual decrease in intensity from the core outwards, typical of elliptical galaxies. A disk component might be present, but it is not a very prominent feature. There are no obvious spiral arms or strong dust lanes visible. There appears to be a mild disturbance in the outskirts of the galaxy, possibly indicative of a minor interaction or tidal feature, but it is not a strong, clear signal of a merger. Color gradients are subtle, with the core potentially exhibiting a slightly yellower hue compared to the outer regions, consistent with an older stellar population. The galaxy appears to be moderately massive, and the star formation rate is likely very low. Overall, this galaxy appears to be a relatively evolved system, possibly undergoing a minor interaction.
