The galaxy presents as a somewhat diffuse object of moderate angular size. It appears to be undergoing some form of disturbance or interaction, possibly related to tidal forces. The overall morphology is not clearly defined as either elliptical or spiral, but the light distribution suggests an irregular structure. There are signs of faint extended features that could be tidal tails or debris from a possible minor merger event. There is a slight color gradient visible, with the central regions appearing redder in comparison to the outer regions which appear greener. No distinct spiral arms or prominent dust lanes are obviously visible.
