The galaxy presents as a somewhat flattened, disk-like structure viewed at a moderate inclination. A bright, concentrated central bulge or core region is evident. There are some hints of spiral arm structures, but they are not sharply defined. A color gradient is visible, with a bluer hue towards the outer edges of the disk suggesting ongoing star formation. The galaxy does not appear to be undergoing any major mergers or significant tidal interactions, although there is a slight distortion of the outer disk which could indicate a minor interaction or disturbance.
