The galaxy presents an elliptical morphology. The light is concentrated toward the center of the galaxy, forming a bright, slightly yellow core. Surrounding this core is a more diffuse halo exhibiting a gradient of color, subtly shifting from yellowish-white at the core's edge to a greenish-blue hue further out. This suggests a possible radial distribution of stellar populations, with older, redder stars concentrated in the center and younger, bluer stars in the outskirts. There is no readily apparent spiral structure or dust lanes visible in this image. The overall impression is that of a relatively smooth and spheroidal system, with some indication of ongoing or recent star formation. There appears to be a slight asymmetrical disturbance along the outer edge of the halo.
