The galaxy presents as a concentrated, elliptical-like structure. A significant fraction of its light is centralized, exhibiting a smooth morphology with a high degree of roundness. The galaxy's light profile suggests a lack of prominent spiral arms or a well-defined disk. There is some indication of potential disturbances or interactions based on the asymmetry in the outer regions, possibly indicative of past minor mergers. The color index appears to be redder overall, pointing to a population dominated by older stars and potentially lower levels of current star formation activity.
