The galaxy presents as a relatively smooth, elliptical-like structure with no immediately obvious spiral arms. The light distribution is concentrated towards the center, suggesting a prominent galactic nucleus. The color profile indicates a population of older stars, and the overall morphology suggests a relatively evolved system that has likely undergone significant merging in the past. There is no clear dust lane. The galaxy is slightly more luminous in the redder wavelengths. There are some small disturbances to the overall smooth morphology.
