The galaxy presents a generally smooth appearance, with minimal discernible internal structure. It exhibits an elliptical shape, elongated along its major axis, appearing somewhat cigar-shaped. The galaxy's light profile is centrally concentrated, with a gradual decrease in luminosity extending outwards from the core. Color gradients are subtle, but the central region appears slightly more yellow/orange, possibly indicating an older stellar population, while the outer regions seem subtly bluer, suggesting the presence of younger stars or ongoing star formation at a low level. There is no strong evidence of significant tidal disturbances or ongoing major mergers, although minor asymmetries cannot be ruled out given the resolution. The galaxy is relatively compact.
