The galaxy appears as a roughly circular, smooth structure, displaying a centrally concentrated luminosity profile that fades gradually towards its outer regions. There is little indication of distinct spiral arms or a prominent disk. The color profile suggests a relatively uniform stellar population, possibly dominated by older stars, as indicated by a subtle reddish hue throughout the galaxy's body. Minor disturbances or faint tidal features are suggested by some irregularity in the outermost regions. The overall morphology appears more consistent with an elliptical galaxy or a lenticular galaxy with a bulge-dominated structure.
