The galaxy appears as a relatively smooth, centrally concentrated object. Its color profile indicates a stronger presence of redder light, with subtle variations in hue across its extent. The morphology suggests a dominant smooth component, with little evidence of spiral arms or other distinct features typically associated with disk galaxies. There is no evidence of any merging or significant disturbances in its structure, indicating a relatively undisturbed state. The overall shape appears more rounded than elongated, though further high-resolution imaging would be required to determine its precise ellipticity. The integrated light of the galaxy suggests it is moderately luminous, exhibiting a population of older, redder stars.
