The galaxy appears to be an elliptical or spheroidal system, exhibiting a smooth, featureless morphology. Its light profile suggests a concentrated central bulge, with luminosity decreasing gradually towards the outer regions. The color is predominantly yellowish-orange. There are no apparent spiral arms, dust lanes, or other distinct features such as tidal tails or strong irregularities to suggest a recent major merger. The galaxy appears largely undisturbed, with a high degree of symmetry. The absence of well-defined features and the smooth light distribution indicates an older stellar population and low ongoing star formation.
