The galaxy presents as a smooth, elliptical structure. It exhibits a concentrated, luminous core, likely indicative of an older stellar population. There are no discernible spiral arms or prominent dust lanes. The outer regions of the galaxy fade gradually, suggesting a relatively uniform distribution of stars. Coloration appears to be generally redder, consistent with a population of evolved stars and a lower rate of active star formation. There is no evidence of ongoing major mergers or significant tidal disturbances affecting the overall morphology. The shape appears generally rounded, with minimal elongation or asymmetry.
