The galaxy appears to be a relatively smooth, elliptical or lenticular type. It exhibits a centrally concentrated luminosity profile, lacking prominent spiral arms or a well-defined disk structure. There is some suggestion of a slight elongation, but the overall morphology leans towards being somewhat round, although possibly in between round and elliptical. The galaxy's color suggests a population of older stars, with a redder hue dominating. There is only very slight suggestion of any ongoing star formation, with no easily visible blue regions or HII regions. The galaxy does not exhibit signs of major mergers or significant tidal disturbances. Some minor disturbance cannot be ruled out.
