This galaxy exhibits a roughly elliptical morphology with a bright, concentrated central bulge that gradually fades into a diffuse outer halo. The color profile suggests a relatively evolved stellar population, with a higher concentration of older stars in the bulge, indicated by the yellowish-white hue. Fainter, bluer regions, suggestive of more recent star formation, are present but not as pronounced, tracing the galaxy's disc shape. The overall structure appears relatively undisturbed, with no obvious signs of ongoing major merger activity, though a possible minor disturbance cannot be ruled out given slight asymmetry. The galaxy's disk has a cigar-like shape.