The galaxy presents a generally smooth morphology with some suggestion of a possible disk-like component. The color distribution appears to be redder in the central region, transitioning to slightly bluer hues in the outer areas. There are no obvious spiral arm structures or bar features discernible.

Based on the color profile and smooth morphology, the galaxy could be an elliptical or lenticular type, though some disturbed features indicate a possible minor merger. A low rate of ongoing star formation seems likely.
