The galaxy presents as a fairly smooth object, with an elliptical morphology. The light distribution appears centrally concentrated, with a bright nucleus that diffuses outward into a less luminous extended halo. The galaxy exhibits a moderate degree of elongation. There is no obvious spiral arm structure or prominent dust lanes visible. The overall color appears relatively uniform across the galaxy, with a hint of a redder hue which is consistent with an older stellar population and a low current star formation rate. The lack of significant morphological disturbance suggests the absence of recent major merger events.
