The galaxy appears to be a relatively smooth, early-type system, likely an elliptical or lenticular galaxy. It presents a centrally concentrated light profile, with a bright, yellowish core that suggests a population of older stars. The galaxy exhibits a slight elongation, but it lacks prominent spiral arm structures. Some subtle bluer patches or faint disk-like features are present in the outer regions, indicating regions of younger, bluer stars. Overall, the galaxy's morphology suggests that it has undergone significant evolution and is possibly in a relatively quiescent phase of star formation. There are no indications of ongoing major mergers or significant tidal disturbances. The faintness of the galaxy indicates it is quite far away.
