The galaxy presents as a somewhat elliptical structure, with a bright, concentrated central bulge. The light distribution suggests a relatively smooth morphology, indicative of an early-type galaxy. There's a subtle elongation, with the apparent major axis extending horizontally in this view. The color profile indicates a generally redder hue, particularly within the central region, which could imply a population of older stars and a lower rate of ongoing star formation. Fainter, diffuse light extends outwards from the central region, gradually fading into the background. No distinct spiral arms or prominent dust lanes are visible. There are possibly minor indications of a faint disk. There does not appear to be any signs of mergers or major tidal disturbances.
