The galaxy presents as a relatively smooth, elliptical morphology. The central region exhibits a high degree of luminosity, indicating a concentrated nucleus. There's a noticeable falloff in surface brightness extending outward from the core, suggesting a lack of significant star formation in the outer regions. The overall color is subtly reddish, indicating a population of older stars dominating the light output. There is a mild hint of a disk but without prominent spiral arms, and with only the faintest structures within it. There is no clear evidence of ongoing mergers or major disturbances affecting the galaxy's structure.