This galaxy appears to be a relatively smooth, elliptical system. It exhibits a high degree of central concentration with a generally round morphology. There may be a hint of a faint, extended halo surrounding the core. The galaxy's color profile indicates a population of older stars, with a redder color index dominating. There is no obvious evidence of spiral arms, dust lanes, or ongoing major merger activity. There might be a hint of minor disturbance or tidal features, potentially indicative of a past interaction or minor merger event. Star formation appears to be relatively quiescent.
