The galaxy presents as a somewhat elongated structure, exhibiting a smooth overall appearance with a central bulge that appears relatively prominent. The central region displays a yellowish-white hue, suggesting a population of older stars. The outer regions show a faint bluish tint, hinting at the presence of younger, hotter stars and possibly ongoing star formation, albeit at a modest rate. There appears to be some evidence of tidal disturbances. The galaxy's shape is noticeably deviate from a perfectly circular morphology.
