The galaxy presents a generally smooth, elliptical morphology. The light distribution suggests a centrally concentrated brightness profile, with the core appearing relatively bright and a gradual decrease in luminosity towards the outer regions. Faint, diffuse extensions are visible at the furthest edges of the galaxy. The object’s overall shape can be described as somewhat rounded.

The galaxy exhibits a color gradient, shifting from a bluer hue at the very center, and trending towards redder colors in the outer regions. This color variation could indicate differing stellar populations, with younger, hotter stars concentrated in the core region and older, cooler stars dominating the outskirts. There is no evidence of well-defined spiral arms or a prominent disk structure; the light appears blended and uniform. There are no signs of any major mergers, though some minor disturbance or irregularities cannot be ruled out, given the limitations of the image resolution.
