The galaxy presents as an elliptical or lenticular system, exhibiting a smooth, largely featureless morphology. The light profile appears concentrated towards the center, with a gradual decline in surface brightness outwards. There is minimal evidence of spiral arm structures or significant dust lanes. The galaxy exhibits a color gradient, appearing somewhat bluer in the outer regions and trending toward redder hues towards the core. The overall shape is approximately elliptical, tending towards a slightly elongated, "in between" form but without distinct cigar-shaped features. There is no discernible evidence of major mergers or significant tidal disturbances. The galaxy is situated at a considerable redshift, indicating a substantial distance. Considering the apparent magnitude and estimated redshift, it is intrinsically luminous. The colors suggest a population dominated by older stars, particularly in the central regions. The galaxy is undergoing a moderate amount of star formation.
