The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The core exhibits a yellow-orange hue, suggestive of an older stellar population. The outer regions display a slightly bluer color, indicating the presence of some younger stars, however, overall star formation rate appears to be low. The galaxy shows no distinct spiral arms or prominent dust lanes. There is no sign of strong tidal disturbances or interactions with other galaxies. The object appears to be a fairly isolated galaxy, likely an early-type galaxy transitioning away from vigorous star formation.
