The galaxy presents as an elliptical or lenticular system, characterized by a smooth, centrally concentrated light distribution. There's a lack of discernible spiral arm structure or prominent dust lanes. The core exhibits a yellowish hue, potentially indicative of an older stellar population. The overall shape is roughly rounded, though some elongation is present. There is no evidence of major disturbances such as tidal tails or disrupted morphology, suggesting it is not currently undergoing a major merger event, but there may be a slight asymmetry. The galaxy appears relatively compact. There may be some low level star formation occurring, but it is mostly quiescent.
