The galaxy presents as a centrally concentrated, elliptical-like structure. It exhibits a smooth luminosity profile, with no readily discernible spiral arms or distinct features such as dust lanes or prominent star-forming regions. The galaxy's color index suggests a population of older stars, giving it a slightly redder hue. The observed ellipticity indicates a shape that is somewhat elongated, but not highly flattened. There might be a minor disturbance in the galaxy’s structure. The galaxy appears to be relatively isolated, showing no clear signs of a major ongoing merger, although subtle disturbances may be present.
