The galaxy presents an elliptical morphology, showing a smooth, centrally concentrated light profile. The galaxy's shape is primarily oblate, though there is some slight elongation in its structure. The central region exhibits high luminosity, suggesting a dense stellar population. The outer regions of the galaxy appear fainter and more diffuse. There are no prominent spiral arms or distinct features indicative of active star formation visible. There are no signs of a major merger or tidal disturbance, although the galaxy's structure does show some irregularity, potentially a minor disturbance or interaction. The galaxy's color suggests a population of older stars, with a subtle shift towards redder wavelengths in the central region.
