The galaxy presents as an elliptical morphology with a smooth, diffuse light distribution. The central region exhibits a concentrated luminosity, transitioning to a fainter halo. The color profile suggests a relatively old stellar population, indicated by the redder hues in the central bulge, with a slight shift towards bluer tones in the outer regions, possibly indicating some recent, albeit limited, star formation. There's no obvious dust lane or spiral arm structure visible. The overall appearance implies that this galaxy has likely undergone significant evolutionary processes, leading to its present spheroidal shape. There is a slight irregular shape visible, possibly a slight disturbance.
