The galaxy presents as a relatively smooth, elliptical structure with a noticeable central bulge. Its overall shape appears elongated, displaying a cigar-like morphology. The light distribution within the galaxy is concentrated towards the center, gradually fading into the outer regions. The color profile is suggestive of an older stellar population, with a generally redder hue. There are no readily apparent spiral arm structures or significant dust lanes visible in the image. Evidence of major mergers or tidal disturbances is minimal, suggesting a relatively undisturbed evolutionary history. Star formation appears to be quiescent, further indicating a dominance of older stars.
