The galaxy presents as an elliptical morphology, appearing largely smooth and spheroidal. There's a concentration of light towards the center, suggesting a distinct galactic nucleus or bulge. Color gradients are subtle, with a slightly bluer hue at the outer edges gradually transitioning to a yellower, more reddish core. This may indicate an older stellar population dominating the central regions. There are no obvious spiral arm structures, or intense star-forming regions visible. Indications of minor disturbance are present, though not easily visible. The overall appearance suggests a relatively evolved system that is not undergoing intense star formation.
