The galaxy presents as an elliptical type, exhibiting a smooth, centrally concentrated morphology. A slight elongation is noticeable, deviating from a perfectly circular shape. The light distribution appears relatively even throughout the galaxy, with a gradual decrease in intensity from the core outwards. There is a hint of a redder central region, possibly indicative of an older stellar population concentrated towards the center. Fainter, bluer light is detected in the outer regions, potentially indicating ongoing or recent star formation. The absence of distinct spiral arms or a well-defined disk structure supports the classification as an elliptical galaxy, exhibiting little signs of tidal disturbances or ongoing mergers.
