The galaxy appears to be an elliptical type, exhibiting a smooth, diffuse light distribution with a centrally concentrated luminosity profile. Its shape is generally round, though there's a slight elongation. There is no presence of any distinct spiral arms or prominent disk structure. Subtle variations in color suggest possible differences in stellar populations across the galaxy, with the central region possibly hosting older, redder stars, and the outer regions showing hints of slightly younger, bluer populations, though any clear difference cannot be determined. The galaxy appears relatively undisturbed, showing no strong signs of an ongoing or recent major merger event. The light distribution gradually fades into the background, indicating no abrupt truncation of its stellar halo.
