The galaxy appears to be an elliptical type, exhibiting a generally smooth and concentrated light distribution. There is a slight elongation to its shape, but overall it appears fairly round. The central region displays a redder hue, possibly indicative of an older stellar population. The outer regions are bluer, suggesting more recent star formation, though this is limited. There are indications of a possible minor interaction or tidal disturbance, with a feature off to the side. It could possibly be a very small satellite galaxy, or tidal debris. The galaxy is not actively undergoing a major merger, but subtle disturbances suggest it may be in the process of accreting material or has experienced a minor merger in the past. The spatial extent indicates that it is a relatively massive galaxy.
