The galaxy presents a spiral morphology, characterized by two prominent spiral arms that emanate from a central bulge. These arms display a loose winding pattern, extending outward from the core region. The bulge appears relatively small compared to the overall disk size. A bar-like structure seems to be present within the central region, although it is not strongly defined. The disk exhibits a slight inclination relative to our line of sight, allowing a partial view of its structure. The galaxy shows some color variation, with bluer regions likely indicating areas of active star formation within the spiral arms, and redder tones concentrated towards the bulge possibly indicating an older stellar population. Overall, there are no major signs of interaction or merging present, however, the spiral arms show minor disturbances in their form.
