The galaxy presents as a relatively smooth, centrally concentrated object. It exhibits a generally elliptical morphology, appearing largely featureless with no immediately discernible spiral arms or a bar structure. The galaxy is approximately round in appearance. There is minimal evidence of any major disturbances or merging activity affecting its overall structure. Color gradients across the galaxy appear subtle, with the central region appearing slightly brighter and potentially more yellow/white than the outer edges, suggesting a possible concentration of older stellar populations towards the center, but there is minimal to no change in color across the object. The color suggests ongoing star formation, albeit at a modest rate. The galaxy appears to be a considerable distance away.
