The galaxy presents a generally smooth, elliptical morphology. It exhibits a centrally concentrated luminosity profile with a gradual decrease in surface brightness towards its outer edges. The core region displays a yellowish hue, suggestive of an older stellar population, while the outer regions appear marginally bluer. No obvious spiral arm structures or significant dust lanes are discernible. There is no clear evidence of a recent or ongoing major merger event, although a slight asymmetry in the outer isophotes hints at a possible minor interaction or disturbance. The overall shape is largely round, with a minor departure towards a more elongated form. Based on the color profile and morphology, the galaxy appears to be a relatively massive system, likely of an early-type classification with a modest star formation rate.
