The galaxy presents a largely smooth, elliptical morphology. Its central region exhibits a high degree of concentration, appearing bright and generally spherical in shape. Moving outward from the core, the light gradually diminishes and fades, appearing to transition into a more diffuse halo. The galaxy appears elongated, as opposed to being perfectly round. There is a subtle indication of a disk-like structure. There is no evidence of strong tidal disturbances or any major ongoing merging activity. The galaxy's overall color is suggestive of an older stellar population, with a redder hue dominating the light emitted. The galaxy shows no signs of significant star formation.
