The galaxy presents as a moderately bright, elliptical-shaped object. It appears to be relatively smooth in texture, lacking prominent spiral arms or distinct features within its structure. There is a concentration of light towards the center of the galaxy, suggesting a dense central bulge or core. The outer regions of the galaxy gradually fade into the background, indicating a diffuse halo. A slight color gradient is observed, with the central regions exhibiting a more yellowish hue compared to the outer edges, which possess a bluer tint. This may suggest an older stellar population in the core and relatively younger population on the outer edges. The galaxy's overall morphology suggests it is undergoing little to no major mergers or disturbances.
