The galaxy presents as a relatively smooth, elliptical-like structure, though not perfectly circular. It appears slightly elongated. The central region exhibits a brighter, more concentrated light, suggesting a prominent galactic nucleus or bulge. The light distribution transitions smoothly from the core to the outer regions, without significant clumping or distinct spiral arms.

Color analysis indicates a dominant yellowish-red hue in the central region, suggestive of an older stellar population and/or significant dust obscuration. The outer regions display a shift toward slightly bluer tints, potentially indicating ongoing, albeit subdued, star formation. There is no indication of a major ongoing merger, however there appears to be a slight irregularitiy in the disc suggesting a possible minor disturbance. Overall, the galaxy’s morphology points towards a system that is well into its evolution.
