The galaxy presents as a moderately luminous, elliptical galaxy with a smooth, featureless morphology. The core exhibits a concentrated luminosity, suggesting the presence of an older stellar population. The color gradient transitions from a slightly redder core to a bluer outer halo. There is a noticeable lack of spiral arm structures or dust lanes. There is no evidence of a significant ongoing merger, though some subtle irregularities may be indicative of a prior minor interaction. The galaxy appears relatively isolated.
