The galaxy appears as a centrally concentrated, elliptical-like structure with a smooth, diffuse light distribution. There is a discernible color gradient, with the central region exhibiting a yellowish-white hue, suggesting a population of older stars. The outer regions of the galaxy fade into a redder color, with no defined spiral arms or prominent dust lanes visible. The galaxy’s shape is somewhat elongated. There is no evidence of a significant tidal disturbance or ongoing major merger activity, although a slight asymmetry suggests the possibility of a minor interaction or disturbance. The galaxy's overall morphology indicates a relatively evolved system, likely dominated by an older stellar population.
