The galaxy appears to be a relatively smooth, elliptical type with a concentrated central bulge. It exhibits a nearly circular morphology, with minimal evidence of a disk structure or spiral arms. There are some subtle features suggesting a degree of recent or ongoing star formation activity, as indicated by the slightly bluer hue toward the central region. The galaxy does not display any obvious signs of major mergers or significant tidal disturbances, though a minor asymmetry or subtle feature might suggest a past interaction. Overall, this galaxy presents as a quiescent system, likely dominated by an older stellar population, though not completely devoid of recent star birth. The estimated size suggests it is a moderate sized galaxy.
