The galaxy presents as a slightly elongated, lenticular-like object with a prominent central bulge. The core exhibits a bright, concentrated luminosity that fades gradually outward, transitioning into a fainter, diffuse halo. There are no prominent spiral arm structures or distinct features indicative of active star formation visible. The overall color profile suggests a predominantly older stellar population, with a subtly redder hue in the core and a bluer tint in the outer regions. The galaxy exhibits minimal signs of significant tidal interactions or morphological disturbances. The overall structure appears relatively smooth and undisturbed.
