The galaxy presents an elliptical morphology with a smooth, centralized luminosity profile. Its shape appears moderately elongated, exhibiting a cigar-like form. The core region shows a high concentration of light, suggesting a dense stellar population. There is a subtle fading of luminosity as one moves outward from the core, transitioning to a less dense halo. No prominent spiral arm structures or significant dust lanes are readily apparent within the image. The overall color is relatively uniform, displaying a slightly yellow-orange hue indicative of an older stellar population, though there is some indication of ongoing, though subdued, star formation. There are no visible signs of recent major merger events, though some minor tidal disturbance cannot be ruled out.
