The galaxy presents as a relatively compact object. Its core appears as a bright, concentrated region. The light distribution around the central bulge indicates a smooth, elliptical morphology. There are no visible spiral arms or prominent dust lanes, reinforcing the categorization as a galaxy that is smooth in appearance.

The galaxy's color profile suggests a redder overall hue, indicative of an older stellar population. The absence of blue regions signifies that the star formation activity is relatively quiescent or non-existent. No apparent signs of tidal tails, shells, or any other morphological disturbances are observed, suggesting that the galaxy is currently not undergoing a major merger event, but there is a hint of some minor irregularities.
