The galaxy presents as a luminous, elliptical morphology with a bright, concentrated central bulge. The overall color index appears relatively red, suggesting a population dominated by older, evolved stars. There is no prominent evidence of spiral arm structures or significant dust lanes within the visible spectrum. The surface brightness profile indicates a smooth, gradual decline from the core outwards, which supports the classification of an elliptical galaxy. Its elongation is moderate, being more of an 'in between' shape rather than perfectly round. There is a subtle asymmetry in the outer isophotes, which could indicate a past minor interaction or accretion event. No obvious signs of active galactic nuclei or ongoing major mergers are directly apparent from the morphology alone.
