The galaxy presents a largely smooth, elliptical morphology. Its color profile indicates a dominance of older stellar populations, with a yellowish-orange hue concentrated towards the core. The light distribution is centrally concentrated, with a gradual falloff in surface brightness moving outwards. There is faint suggestion of a slight elongation, but the overall shape is fairly rounded. No distinct spiral arm structures or significant dust lanes are apparent. The galaxy appears relatively undisturbed, with no clear evidence of recent major merger activity. Faint blueish colors are present in the outer edges of the galaxy, potentially implying the presence of younger stars or active star formation in these regions. Based on these characteristics, the galaxy likely represents a relatively massive system with a high degree of stellar population aging and an ongoing, but low, rate of star formation.
