The galaxy presents as a relatively small, faint object. Its morphology appears to be disk-like, though lacking well-defined spiral arms, and it exhibits a smooth or featured appearance, with neither being particularly dominant. There is some indication of possible interaction or minor disturbance with a distorted arm or merging feature. The galaxy has an apparent color gradient, appearing bluer toward the center and redder in the outer regions. This could indicate older stellar populations dominating the outskirts, while more recent star formation is occurring in the central region.
