The galaxy presents a largely smooth morphology with a slightly elliptical shape. It displays a concentration of light towards the central region, indicating a prominent galactic nucleus. The overall color profile suggests a population of older stars, potentially with a relatively low rate of ongoing star formation. There is a subtle hint of a disk-like structure but no strong spiral arms are evident. The galaxy shows no obvious signs of major mergers or significant tidal disturbances, although a minor interaction cannot be entirely ruled out based on the slight asymmetries observed.
