The galaxy appears to be a relatively small, elliptical galaxy, displaying a smooth, concentrated light profile. Its shape is more in between a circle and cigar than completely round. There is little to no evidence of spiral arms or a distinct disk structure. The galaxy's color is predominantly a slightly warm, suggesting a population of older stars. The absence of strong blue colors indicates a low rate of ongoing star formation. There appears to be no significant signs of interaction or merging activity with other galaxies, though a minor disturbance cannot be fully excluded. The galaxy is relatively isolated in the observed field.
