The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The light distribution indicates a gradual decline in luminosity from the core outward. The color profile suggests an older stellar population, with a yellowish-white hue dominating the central regions, potentially indicative of a lack of active star formation. There's a hint of bluer coloration towards the edges of the galaxy, possibly signifying the presence of younger stars in these regions, though faint. The galaxy displays an elongated shape, with the major axis extending significantly further than the minor axis. No significant spiral arm structures or dust lanes are discernible in the image. There's no obvious evidence of strong tidal disturbances or interactions with other galaxies in the immediate vicinity. The overall morphology indicates a system that has likely undergone significant evolutionary processing, potentially merging and settling into its current form. The size appears to be moderate, neither exceptionally large nor particularly compact, given the implied distance.
