The galaxy presents an overall smooth and elliptical morphology, suggestive of an early-type galaxy, possibly an elliptical or lenticular galaxy. The central region exhibits a bright, diffuse glow, which decreases gradually towards the edges. There is a slight elongation observed in the galaxy's shape, but it appears largely rounded. Faint hints of a possible disk structure can be seen. No distinct spiral arms or strong dust lanes are discernible. There may be a slight disturbance in the galaxy's shape. Redder hues are observed in some regions of the galaxy, possibly indicating older stellar populations or dust. There seems to be some minor merging activity. The galaxy appears relatively isolated in the image.