The galaxy presents an elliptical morphology, exhibiting a smooth, concentrated distribution of light. The core region is characterized by high luminosity, indicative of a dense stellar population, potentially an aging population. A gradual decrease in luminosity is observed as one moves outward from the center, lacking the distinct spiral arm structures often associated with disk galaxies. It appears that the shape tends more to a spherical form than a flattened disk. There is no visible evidence of major mergers or tidal disturbances, however, this should be investigated with more powerful instrumentation. The integrated light suggests older stellar populations and potentially lower rates of current star formation, with an overall redder color index dominating the core.
