The galaxy presents as a largely smooth, elliptical-like object, with a concentrated central bulge. It exhibits a gradual decline in luminosity from the core outwards. There is little to no apparent spiral structure or distinct features, and it seems to be relatively undisturbed, with no major signs of ongoing merger activity. The color profile indicates a higher concentration of older stellar populations, with redder hues dominating the central region, gradually fading to a bluer tinge in the outskirts. This suggests a lower rate of current star formation and an older stellar population is dominating the mass of the galaxy. The overall morphology is indicative of a mature system.
