The galaxy appears to be a relatively smooth, elliptical galaxy with a concentrated central bulge. Its overall shape is generally round. The light from the galaxy is dominated by older stellar populations, indicated by the yellowish hue of the central bulge, with some bluer stars in the outer regions. There is no evidence of prominent spiral arms or significant dust lanes. The galaxy does not appear to be undergoing a major merger or exhibiting strong tidal features. Some minor disturbances may be present but are not obvious, suggesting the possibility of a past interaction or accretion event.
