The galaxy presents as a smooth, elliptical form with a centrally concentrated bulge. The light profile appears to gradually diminish from the core outwards, exhibiting no distinct spiral arms or prominent features. The overall color is a pale yellowish-white, suggesting an older stellar population. The galaxy's shape is noticeably elongated. There is no evidence of significant dust lanes or ongoing major merging activity. Minor disturbances are a possibility, however there is no clear evidence for this in the image.
