The galaxy presents a largely smooth and elliptical morphology. It exhibits a concentrated central bulge region that appears yellow and diffuse, indicating a population of older stars with less ongoing star formation. The overall color suggests a relatively low rate of star formation and a dominant population of older, redder stars. There is a hint of a fainter, bluer, disc-like component surrounding the bulge, though this is not particularly pronounced and the resolution prevents detailed morphological classification. The galaxy does not obviously display any strong tidal features, indicating it is likely not undergoing any major mergers currently, however a possible minor disturbance is not ruled out. The shape of the galaxy is generally round, with no major elongations or cigar-like features.
