The galaxy presents an elliptical morphology, exhibiting a smooth, centralized light distribution. Its overall shape appears moderately elongated, verging towards a cigar-like form. The central region displays a pronounced concentration of light, suggesting the presence of a significant bulge component. There are no readily discernible spiral arms or significant dust lanes visible in the image. The galaxy appears relatively undisturbed, showing no strong signs of ongoing or recent major merging activity. A subtle, faint halo surrounds the central body, gradually fading into the background.
