The galaxy appears as a single, relatively compact object. Its morphology is generally smooth, with a high degree of symmetry. The color profile suggests a population dominated by older stars, exhibiting a reddish-yellow hue. There are no prominent spiral arms or a well-defined disk structure visible. A slight central concentration of light suggests the presence of a galactic bulge. No signs of ongoing or recent major mergers, or significant tidal disturbances are present. The shape appears somewhere between round and elongated. Star formation appears to be low in the galaxy.
