The galaxy presents a generally smooth morphology, with a high degree of central concentration. It appears elliptical or lenticular in shape, exhibiting a noticeable elongation. There is a discernible color gradient, with the central region appearing more yellow/gold, transitioning to a bluer hue in the outer regions. Although the majority of the galaxy is smooth, there is a faint hint of a disk component within the galaxy and the possibility of small disturbance or tidal feature is not discounted. The general color profile suggests a evolved population of stars within the central bulge, potentially older and metal-rich, while the outer regions may contain more active star formation regions with younger, bluer stars. The galaxy has estimated to be a moderate mass galaxy.