The galaxy presents as a single, somewhat amorphous object with a centrally concentrated luminosity profile. The core region exhibits a smooth, nearly spherical morphology, suggesting a dominance of older stellar populations. Moving outward from the core, the light gradually decreases in intensity, fading into a poorly defined edge. There is little evidence of significant spiral arm structure or dust lanes, further reinforcing its characterization as an elliptical-type galaxy, or perhaps a lenticular galaxy seen at an inclination where disk features are obscured. Slight colour variations are noted from the core outward, implying the presence of low-level star formation, or possibly a population gradient in the stars. There is no evidence of ongoing major merger activity. Minor disturbances or tidal features are not readily apparent.