The galaxy presents as a moderately bright object with a notable elliptical morphology. The light distribution appears relatively smooth across the galaxy's body, indicative of an evolved stellar population. There may be some subtle features suggesting minor disturbances or interactions. Its color profile seems redder than average in the DESI g, r, and z bands, which is consistent with older stars, and there may be evidence of ongoing but subdued star formation, though the specific star formation rate appears low. The galaxy's projected size on the sky is relatively small, placing it at a moderate distance from our line of sight. Analysis suggests a substantial stellar mass.
