The galaxy presents as a relatively smooth, elliptical-like structure with a centrally concentrated brightness profile. The light distribution appears somewhat diffuse. There is a slight elongation, and some asymmetry suggesting possible minor gravitational disturbance. The galaxy exhibits a yellowish hue, indicative of an older stellar population and potentially lower current star formation activity. The galaxy is compact in size, estimated to be around 6 kiloparsecs in diameter. There appears to be a subtle color gradient, with the central region possibly slightly redder than the outer regions. A merging event is possible, however the galaxy more likely shows signs of tidal disruptions.
