The galaxy presents as a single, mostly smooth object. It exhibits a generally elliptical morphology, appearing mostly round with a slight elongation. The galaxy's light distribution is concentrated towards the center, with a notable yellow-orange hue in the core, suggesting a population of older stars. The outer regions fade in intensity, displaying a broader, less defined boundary. Subtle color variations, trending toward redder tones, can be discerned in patches within the outskirts. The lack of distinct spiral arms or prominent dust lanes indicates the possibility of it being an elliptical galaxy, or a spiral galaxy with a very small disk or a disk seen face-on. There is no clear indication of any major ongoing mergers or significant tidal disturbances affecting the galaxy's structure, though minor irregularities cannot be ruled out at this resolution.
