This galaxy exhibits a predominantly smooth morphology, with a concentrated central bulge displaying a yellowish hue, potentially indicative of an older stellar population. A faint disk structure is suggested, although the arms are not well-defined. The overall shape is elliptical. There is a suggestion of a minor disturbance, possibly due to a past interaction or merger event, given the asymmetry in the light distribution. The galaxy appears relatively isolated, without any immediate signs of major mergers or significant tidal interactions. A high degree of roundness is observed.
