The galaxy presents as a centrally concentrated object, with a primarily smooth morphology. It exhibits a slightly elongated shape, appearing more "in-between" round and cigar-shaped. The core region displays a bright, yellowish hue, suggesting a significant population of older stars. A fainter, blueish halo surrounds the core, potentially indicating the presence of a younger stellar population within the outer regions. There is a faint hint of what could be very subtle disturbances or faint, diffuse features extending outward from the main body. There is no obvious spiral structure, and no evidence of a major ongoing merger. The overall impression is that of a relatively undisturbed galaxy transitioning to a quiescent state.
