The galaxy presents as a relatively smooth, centrally concentrated object. The shape is generally elliptical, displaying a slight elongation but not a strong disk-like feature. There appears to be no clear spiral arm structure or bar. The core exhibits a higher intensity, suggesting a concentration of older stars. Faint outer regions are visible around the central core, these areas suggest a larger distribution of stars with lower surface brightness, possibly a stellar halo. Overall, the galaxy appears to be relatively undisturbed, although a minor asymmetry is potentially observable. The color suggests a population of older stars, with a possible low level of ongoing star formation, resulting in a slightly bluer color than expected.
