The galaxy presents an overall smooth morphology, with an elliptical appearance. The central region is characterized by a concentrated, bright, yellowish core which gradually diffuses outwards. Moving from the core outward, the color transitions to a less saturated, fainter yellow-green halo. The overall structure suggests a relatively old stellar population, particularly concentrated towards the center. There are no visible spiral arm structures, nor are there any obvious signs of strong tidal disturbances or a recent major merger event; however, there is minor asymmetry in the outer halo which may be indicative of a past interaction.
