The galaxy presents as a relatively smooth, centrally concentrated object. The light distribution suggests a flattened spheroid, tending more towards a slightly elongated shape than a perfect circle. There's a discernible gradient from a bright, high-surface-brightness core to a fainter, extended halo. There is some indication of a possible disk structure, though not sharply defined, with hints of fainter, diffuse arms or tidal features extending from the central bulge. No prominent dust lanes are visible. The dominant color appears yellowish-white, likely indicative of an older stellar population, although with some slight mottling, perhaps suggesting areas of recent low-level star formation. There are no indications of a major ongoing merger, or an active galactic nuclei.
