The galaxy exhibits an overall smooth morphology, though with subtle features suggesting some level of disturbance. The light distribution appears centrally concentrated with a noticeable extension in one direction, giving it a somewhat elongated shape. The galaxy appears to be in some sort of interaction. There is evidence of possible tidal tails or bridges, indicating a gravitational interaction with another galaxy or past merger event. The galaxy's color is generally consistent with an older stellar population, though there are regions of bluer light, potentially indicating areas of ongoing star formation, however faint. The shape is somewhere between round and elongated. The overall estimated size suggests a relatively large galaxy. The low star formation rate and high mass suggest that this is a mature system.
