The galaxy presents an elliptical morphology, though exhibiting some potential disturbed features indicative of possible past or ongoing interaction. The light distribution suggests a central, bright bulge with a notable color gradient. The core region appears comparatively blue-white, possibly reflecting younger stellar populations. Moving outward, a region displays a more yellow-red color, indicating the presence of older stars or dust obscuration. The morphology leans towards an "in between" roundness classification, not perfectly spherical or elongated. There is some visual evidence of a minor disturbance in the structure, such as tidal tails. Overall the galaxy exhibits characteristics somewhere between a pure elliptical and a spiral, potentially a transitional form or a result of a recent merger.
