The galaxy appears as a centrally concentrated object with a smooth, diffuse halo extending outwards. The core displays a yellowish hue, possibly indicative of an older stellar population. There is evidence of bluer regions within the galaxy, located slightly off-center, suggesting localized areas of more recent star formation. The overall shape appears close to round. There are faint traces that hint at possible minor disturbances in the galaxy's structure, though these could also be attributed to image noise or artifacts. The galaxy does not appear to be undergoing a major merging event, but the slight asymmetries could indicate a minor interaction in its past.
