The galaxy presents as a moderately luminous object, exhibiting a generally smooth morphology. The light distribution appears concentrated towards the center, suggesting a significant bulge component. The overall shape is somewhat elliptical, displaying a slight deviation from perfect circularity. There are no discernible spiral arm structures or prominent dust lanes visible in the image. The galaxy's color index suggests a moderately red population, possibly indicating a relatively older stellar population with ongoing but subdued star formation. There is no clear evidence of strong tidal interactions or merging activity.
