The galaxy presents an elliptical morphology, appearing somewhat rounded but with slight irregularities in its overall shape. A central, bright core dominates the galaxy's structure, exhibiting a yellowish hue, potentially indicating an older stellar population and minimal ongoing star formation in the galactic nucleus. Diffuse, reddish regions are observed in the outer edges of the galaxy, possibly indicating the presence of dust lanes or areas of low-level star formation. A distinct tail or arm structure is not visibly present in the galaxy image, but there are hints of some disruption of the regular shape. The galaxy appears to be undergoing some form of interaction, or recent interaction, which has resulted in some minor morphological disturbances. There is no obvious disk structure.
