The galaxy presents as a slightly elongated, diffuse object with a centrally concentrated luminosity. It exhibits a smooth, featureless morphology, lacking any discernible spiral arms or distinct substructures. The color profile appears relatively uniform across the galaxy, tending toward redder hues. This suggests a dominant population of older stars and a relatively low rate of ongoing star formation. The overall shape can be described as somewhere between round and elliptical. There is no clear visual evidence of any major mergers or significant disturbances within the galaxy's structure. 
