The galaxy appears as a single, relatively smooth object with a moderate degree of central concentration. The light profile suggests an elliptical morphology, leaning towards being somewhat rounded rather than elongated. The galaxy exhibits a color gradient, with the central region appearing distinctly bluer than the outer regions which are more yellow. This color difference may be indicative of a centrally concentrated population of younger, hotter stars, while the outer regions are likely dominated by older, cooler stellar populations. There is no obvious evidence of spiral arms, a prominent disk structure, or major tidal disturbances. There are no other apparent irregularities to suggest that it is currently undergoing a major merger event. It might be interacting with the smaller galaxy to its left.
