The galaxy presents a generally smooth morphology, appearing largely featureless and spheroidal in shape. There may be a slight elongation, but the overall form leans toward a more circular, elliptical structure. Its light is concentrated towards the center, exhibiting a strong central bulge. This central region is characterized by a yellowish hue, which could indicate an older stellar population dominating the core. The light gradually fades as it extends outward from the center, suggesting a decrease in stellar density with increasing radius. Faint hints of bluer hues in the outer regions might suggest the presence of some younger, star-forming regions, though these are not prominent. There is no apparent disk structure, spiral arms, or significant dust lanes visible.
