The galaxy presents an elliptical morphology, appearing mostly smooth with a high degree of central concentration. The galaxy exhibits a slightly elongated shape, trending towards an intermediate, non-circular form. A bright, compact core is visible, likely containing an older stellar population, judging by the color gradient transitioning towards redder hues in the nucleus. Moving outward from the core, the galaxy displays a subtle disk-like structure characterized by a bluer color, suggesting the presence of some younger stars, though star formation activity appears relatively low overall. There is no apparent evidence of major ongoing mergers or significant tidal disturbances. Minor irregularities or asymmetries in the outer regions may indicate past interactions or internal processes, but the overall structure indicates it's a fairly relaxed system. The apparent size of the galaxy is relatively small, likely due to its distance.
