The galaxy appears as a centrally concentrated, ellipsoidal object, displaying a smooth morphology. The light profile suggests a prominent bulge component with a gradual fall-off in intensity towards the outer regions. The color distribution indicates a dominant population of older stars in the central region, with a shift towards slightly bluer hues in the outer disk. This could imply ongoing, albeit modest, star formation activity in the outer regions. There is no strong evidence of spiral arms or a well-defined disk structure, but a slightly flattened shape is observed. The galaxy appears relatively isolated, with no obvious signs of major tidal disturbances or ongoing mergers.
