The galaxy presents as a somewhat elliptical, disk-like structure with a relatively smooth and centralized concentration of light. The core region exhibits a pronounced yellowish hue, suggesting a population of older stars or significant dust obscuration. Fainter, bluer regions extend from the main body, indicating regions of more recent star formation. These regions do not present well defined spiral arms. The galaxy is not perfectly symmetrical, exhibiting a slight elongation and a possible minor disturbance. Overall, the galaxy does not appear to be actively merging, although there are hints of potential tidal features or asymmetries in the outer regions, as seen from a possible merging event. The size of the galaxy appears to be of moderate scale.
