The galaxy presents a largely smooth, elliptical morphology. The light distribution is centrally concentrated, exhibiting a gradual decrease in surface brightness from the core outwards. There is a subtle color gradient, trending from a yellower hue in the central region towards a redder color in the outskirts. No distinct spiral arm structures or prominent dust lanes are discernible. There is no evidence of any tidal disturbances or ongoing major mergers and shows an undisturbed morphology. The light distribution suggests an absence of significant ongoing star formation within the galaxy.
