The galaxy presents a generally smooth, elliptical morphology. It appears to be relatively undisturbed with a smooth light profile. The central bulge exhibits a bright, concentrated luminosity, potentially indicating a high density of older stellar populations. Moving outward from the core, the luminosity decreases gradually. The overall shape is somewhat elongated, approaching a cigar-like appearance, but with a dominant, rounded core. Subtle color variations exist across the galaxy, with the central regions appearing more yellowish, potentially suggestive of older stars, while the outer regions exhibit hints of bluer hues. This observation may indicate some low-level ongoing star formation within the galaxy.
