This galaxy appears to be a relatively smooth, elliptical type. It exhibits a centrally concentrated light profile, with the majority of its luminosity emanating from the core region. There's a gradual decrease in light intensity moving outwards from the center, forming a diffuse halo. The galaxy does not appear to have prominent spiral arms or a well-defined disk structure. Its overall shape is closer to round than elongated, with no obvious distortions indicating a major ongoing merger. There is some subtle irregularity along its edges, possibly indicating a minor gravitational interaction or disturbance. The galaxy's color suggests a population of older stars, appearing slightly redder in comparison to galaxies with significant ongoing star formation. The overall size appears to be relatively compact.
