The galaxy presents as a centrally concentrated object with a generally smooth morphology. There is little evidence of spiral arm structure or significant dust lanes. The light distribution suggests a dominant bulge component, with a gradual decline in surface brightness outwards from the core. The overall shape is slightly elongated, but appears relatively round. There is no visually discernible evidence of ongoing major merger activity, or major tidal disturbances. The galaxy exhibits a color gradient, appearing more yellow/orange in the central regions, transitioning to slightly bluer hues in the outer regions, suggesting the presence of younger stellar populations there, though this is not very pronounced. The apparent lack of strong features suggests that it is a relatively quiescent galaxy, potentially an elliptical or lenticular type galaxy.