This galaxy presents a generally elliptical morphology. The light profile appears smooth and centrally concentrated, with a gradual decrease in intensity towards the outer regions. Color gradients suggest a relatively homogeneous stellar population, though subtle variations exist. A slight reddening of the color is visible in the periphery in two regions. Overall, there is no strong evidence of spiral arms, a central bar, or significant dust lanes. There are some signs of minor disturbances in its outer regions, suggesting a past or ongoing interaction. The galaxy exhibits an approximately round shape and a smooth texture. There may be a faint disk. 
