The galaxy presents as a spiral, viewed at a shallow angle, not quite face-on. A substantial bulge is visible at its core, exhibiting a yellowish hue, suggestive of an older stellar population. Fainter spiral arms extend outwards from the central bulge, hinting at ongoing star formation within the disk. These arms appear somewhat flocculent and are not sharply defined. The galaxy does not appear to be undergoing any major merger events or significant disturbances based on visual inspection. There may be some subtle indications of a bar structure present, but further data is needed to confirm this assessment. The spiral arms exhibit a moderate winding pattern. Based on color and shape, the galaxy appears to be a disk galaxy with a relatively high stellar mass.