The galaxy presents as a centrally concentrated, luminous object. Its overall morphology appears largely smooth, exhibiting a high degree of radial symmetry. The light distribution suggests a spheroidal component dominates, with minimal evidence of spiral arms or a prominent disk. The elliptical shape is slightly rounded. There appears to be minimal signs of tidal disturbances or ongoing major merger activity with other galaxies. The color profile exhibits a tendency towards redder hues, suggestive of an older stellar population. The galaxy’s estimated size is a few kiloparsecs in radius. Star formation rates seem to be moderate to low. The galaxy is a high-mass object.
