The galaxy presents as a single, relatively smooth object with a concentrated central bulge. The color profile suggests a dominant population of older stars, with a yellowish hue to the central region. The light profile appears fairly symmetrical, lacking any prominent spiral arms or distinct morphological features. There may be a slight extension or faint tidal tail visible to the south, potentially indicating a minor gravitational interaction. The galaxy's overall roundness suggests a classification leaning towards elliptical, though a flattened, disk-like structure cannot be ruled out entirely due to image limitations. Star formation activity appears to be relatively low, based on the overall color and lack of bright blue regions indicative of young, massive stars. There is no evidence of a major ongoing merger, though subtle disturbances might be present. The estimated size and luminosity suggest this is a galaxy of substantial mass.
