The galaxy presents as a predominantly elliptical morphology, exhibiting a smooth, featureless appearance without discernible spiral arms or a prominent disk structure. Its overall shape is approximately round. The color profile suggests a dominant population of older stars, contributing to its reddish-yellow hue. There is no obvious evidence of ongoing major merging activity or significant tidal disturbances. The galaxy appears to be relatively quiescent in terms of star formation activity. The estimated size indicates that the galaxy is moderate in physical extent. The inferred mass suggests a substantial galaxy with a correspondingly high luminosity.
