The galaxy exhibits a roughly elliptical morphology, though with noticeable disturbances suggesting a potential ongoing or recent interaction. There appears to be a prominent central bulge which is surrounded by a less concentrated disk. The disk structure isn't well-defined, indicating that if spiral arms are present, they are not tightly wound or well-formed. Color gradients across the galaxy suggest variations in stellar populations. The core shows a yellowish hue, consistent with older stellar populations. The outer regions display a bluer tint which would indicate some ongoing star formation, even if that rate may be low. The irregular shape of the galaxy along its edges suggests that it may be interacting or undergoing a merger.
