The galaxy presents a generally elliptical morphology, appearing somewhat elongated but predominantly rounded in form. It exhibits a centrally concentrated bulge, luminous and yellowish-white in color, which suggests an older stellar population. Fainter, bluish-white regions extend outwards from the central bulge, indicating the presence of some younger stars and possibly ongoing, but relatively low star formation activity within a disk-like structure. Subtle disturbances or asymmetries might be present in the outer regions, potentially hinting at minor gravitational interactions or past merger events, though these features are not overtly pronounced. There is not much evidence of spiral arm structure. Overall, the galaxy's light profile appears relatively smooth, suggesting a mature system with limited active star formation. The galaxy is located at a considerable distance, as its redshift indicates, approximately 10% the speed of light. This indicates a moderately massive galaxy with a relatively low specific star formation rate.
