The galaxy presents a generally smooth morphology, appearing elliptical in shape. The central region exhibits a higher surface brightness, transitioning to a more diffuse halo at the periphery. The core is noticeably yellowish, suggesting an older stellar population and a relative lack of ongoing star formation. Faint, extended features possibly indicative of tidal interactions or minor disturbances are subtly visible in the surrounding halo. The overall structure appears relatively undisturbed, showing no clear evidence of a major merger event, though the presence of some subtle asymmetries cannot be ruled out. The light distribution is centrally concentrated, tapering off smoothly without distinct spiral arm features or prominent dust lanes.
