The galaxy presents as a centrally concentrated, luminous object with a generally smooth appearance. Its morphology indicates a high degree of radial symmetry, with an elliptical or spheroid-like shape. There is a distinct lack of observable spiral arm structures or significant dust lane features. The color profile is primarily reddish-yellow, with some subtle bluer gradients detectable in the outer regions, suggesting a mix of older stellar populations and perhaps some ongoing, albeit relatively low, star formation. No evidence of significant tidal disturbances or merging activity is readily apparent in this observation. The overall morphology leans towards a quiescent, spheroidal galaxy type.
