The galaxy presents a largely smooth morphology, appearing as a concentrated spheroid. There is a slight asymmetry in the outer regions of the galaxy, hinting at potential minor disturbances. The galaxy exhibits a somewhat round profile. The color gradient shifts from yellow at the core to a bluer hue in the less concentrated regions, potentially suggestive of a small degree of ongoing star formation. The galaxy lacks any obvious spiral arms or a prominent disk. Overall, the galaxy appears to be a relatively quiescent system with minimal ongoing merging activity.