The galaxy presents an elliptical morphology, with a smooth and diffuse appearance. The light distribution suggests a central bulge that diminishes gradually outwards. There is no evidence of spiral arms or a distinct disk-like structure. The galaxy appears to be relatively isolated, showing no signs of major mergers or significant tidal disturbances, though some minor disturbance cannot be ruled out. The color profile indicates a population of older stars, consistent with a relatively quiescent star formation rate. There is no indication of strong ongoing star formation or dust lanes. The galaxy is moderately sized and is located at a considerable distance, as indicated by its redshift.
