The galaxy presents as a roughly elliptical, smoothly distributed luminous object. The core of the galaxy exhibits a bright, concentrated glow, suggesting a high density of stars or an active galactic nucleus. Progressing outward from the core, the luminosity gradually decreases, with a bluish hue in the outer regions. This color may indicate a population of younger, hotter stars. The overall morphology appears relatively undisturbed, lacking any prominent spiral arms or obvious signs of ongoing major mergers or tidal interactions. The shape is moderately elongated, suggesting a possible transition between elliptical and lenticular morphologies.
