The galaxy presents a generally smooth appearance. It exhibits an elliptical morphology, being neither perfectly round nor highly elongated, tending towards an in-between form. There is a suggestion of a possible minor disturbance in its structure. The galaxy has a fairly concentrated center, with a gradually decreasing luminosity outwards. A faint extension or tail-like feature emerges from one end, which may indicate some tidal interaction, although the dominant impression is one of relative isolation and internal coherence.
