The galaxy appears to be a spiral type. Its light is most concentrated at the center and decreases toward the outer edges, creating a diffuse halo. The color profile suggests an older stellar population, which would imply relatively low star formation activity, consistent with the image showing no visually prominent knots indicative of active star forming regions. There is a slight color gradient from the center outwards, with the core being a more yellow/orange than the bluer spiral arms. The morphology suggests the galaxy is relatively undisturbed with no obvious signs of recent major mergers, though there may be some minor asymmetries suggesting possible past interactions. The elongated shape indicates it is being viewed at an angle. 