The galaxy presents as a relatively smooth, elliptical-like structure, with a concentrated central bulge. The light appears to diminish gradually from the core outwards. There may be a faint disk present as indicated by the slight elongation and flattening along one axis, but this feature is not particularly distinct. The color profile suggests a population dominated by older stars, indicated by a yellow-red hue near the center, transitioning to bluer tones in the outer regions which suggests star formation is taking place. No major disturbances or tidal features are immediately apparent, suggesting a relatively isolated system without recent major merger events.
