The galaxy presents as a relatively compact object with an elliptical morphology. The core exhibits a bright, concentrated luminosity profile, with a yellowish tint, indicating a high density of older stellar populations. Moving outwards, the disk component is subtly visible, displaying a slightly bluer hue suggesting the presence of younger stars and possible ongoing star formation. There are hints of disturbances, particularly along the galaxy's plane, potentially indicating tidal interactions or past mergers. The galaxy’s overall structure appears relatively smooth but not perfectly uniform.
