The galaxy presents as a somewhat elongated, elliptical-like structure with a noticeable color gradient. The central region exhibits a concentration of reddish-orange light, suggesting a population of older stars and/or dust obscuration. The outer regions appear fainter and show hints of bluer light, possibly indicating the presence of younger stars. The overall morphology appears relatively smooth, without any obvious signs of strong spiral arms or major disturbances, although a slight asymmetry cannot be ruled out due to the image resolution. The galaxy does not seem to be undergoing any major merging activity, but there may be slight disturbances present. It has an estimated effective radius of approximately 9.5 kpc, assuming a redshift of around 0.26. Considering the colors and morphology, this galaxy could be classified as an early-type galaxy with a moderate stellar mass and star formation rate.
