The galaxy presents as a relatively smooth, elliptical structure with a concentrated central bulge. The core exhibits a reddish hue, potentially indicating an older stellar population or significant dust obscuration. Moving outward from the core, a subtle transition to greenish-blue is observed, possibly suggestive of recent, low-level star formation activity. The overall morphology appears largely undisturbed, lacking strong evidence of ongoing major mergers or tidal interactions, though a slight asymmetry and some minor disturbances cannot be ruled out. The galaxy's shape appears to be somewhere between round and elongated. The presence of a faint, diffuse halo is suspected, contributing to the overall size.
