The galaxy presents an elliptical morphology, exhibiting a smooth and centrally concentrated light distribution. The core region appears bright and yellowish-orange, suggesting an older stellar population is dominant. The galaxy gradually fades outward from the center, with the outer regions exhibiting a slightly bluer tinge indicating the presence of some younger stars, though not significantly prominent. There are hints of subtle disturbances in the outer regions, possibly suggestive of past minor interactions. Overall, the galaxy appears to be a relatively undisturbed elliptical system at a considerable distance, showing evidence of ongoing, albeit relatively low, star formation.
