The galaxy presents as a spiral galaxy, viewed at an angle that is neither face-on nor edge-on. A central bulge appears prominent and concentrated, with a bright yellowish-white hue, suggesting an older stellar population. Fainter spiral arms extend outwards from the central bulge. These arms display bluer regions indicating ongoing star formation. There is no obvious sign of a strong bar structure. The galaxy appears relatively isolated with no signs of major interaction or merging events.