The galaxy appears as a moderately bright, slightly elongated object. It exhibits a relatively smooth, featureless morphology with a central bulge that transitions smoothly into a more diffuse halo. There's an indication of a possible disk-like structure, but it's not well-defined. The color gradient suggests a centrally concentrated stellar population, becoming bluer in the outer regions. No distinct spiral arms or bar structures are discernible in this image. The overall appearance suggests a galaxy with a significant population of older stars, though some ongoing star formation may be present. There are no obvious signs of any major mergers or tidal disturbances.