The galaxy presents as a centrally concentrated object with a generally smooth morphology. There are hints of weak disklike structure. The overall color profile suggests an evolved stellar population, with a redder hue dominating. There is a noticeable absence of distinct spiral arms or prominent star-forming regions. The shape appears mostly round. The galaxy appears isolated, with no obvious signs of major tidal interactions or ongoing mergers. Faint irregularities may be present, suggesting minor gravitational disturbances.
