The galaxy presents as an edge-on spiral, exhibiting a prominent, centralized bulge. The bulge appears smooth and concentrated, with a slightly boxy morphology. The disk is viewed nearly perfectly edge-on, making it difficult to discern any spiral arm structure. It's quite thin, showing a slight warp. The galaxy exhibits a color gradient, with the central bulge appearing yellower, suggestive of older stellar populations. Fainter, bluer light is present in the outer regions of the disk, hinting at ongoing star formation in those areas. No significant dust lanes are readily apparent, though there is some obscuration of the bulge. No obvious signs of any recent or ongoing major merger events are detected, although there may be minor irregularities present in the disk structure, potentially indicative of minor interactions or internal processes. Overall, this galaxy appears to be a relatively undisturbed spiral with ongoing, albeit moderate, star formation. The galaxy is somewhat large and fairly massive.
