The galaxy exhibits a generally smooth morphology, with a predominantly elliptical shape. The central region presents a bright, concentrated luminosity, suggesting a significant stellar population density. The color profile appears to transition from a yellowish-white core towards a more reddish hue in the outer regions of the galaxy, possibly indicating a shift from younger, hotter stars in the core to older, cooler stars in the halo. While the overall structure is largely undisturbed, there are subtle hints of asymmetry or slight irregularities in the outer regions, perhaps caused by a minor gravitational interaction or internal dynamic processes. No distinct spiral arms or prominent dust lanes are visible. The galaxy's apparent color suggests a likely redshift, positioning it at a considerable distance.
