The galaxy presents as a relatively smooth, elliptical morphology. There is a concentrated central bulge that is yellowish in hue, suggestive of an older stellar population. Moving outwards from the core, the galaxy exhibits a diffuse halo with a bluer color gradient compared to the center, suggesting a more recent episode of star formation in the outer regions, although this activity appears to be low. The overall shape is somewhat elongated but not significantly cigar-shaped. There is no obvious indication of major mergers or tidal disturbances; instead, the galaxy appears relatively undisturbed, with a fairly regular structure.
