The galaxy presents as a somewhat face-on spiral with a moderate degree of central concentration. The galaxy exhibits a relatively smooth overall appearance, with a somewhat elliptical shape. Its color profile suggests ongoing star formation, particularly prominent in the central bulge and inner spiral arm regions. There is a slight indication of disturbance in the structure, possibly the result of a minor interaction or internal dynamic processes. No strong bar structure is discernible. The galaxy does not appear to be undergoing a major merger, but minor disturbances cannot be ruled out based on the visual inspection.
