The galaxy appears as a centrally concentrated object with a generally smooth morphology. It presents a relatively symmetrical, elliptical shape. There is no clear evidence of a spiral arm structure, prominent dust lanes, or a distinct galactic bulge. The galaxy exhibits a color gradient, with a bright, almost stellar-like core that appears bluer compared to the more diffuse, redder outer regions. This color variation may be due to differing stellar populations, with younger, hotter stars concentrated in the central region. There are some faint, reddish areas in the surrounding space close to the galaxy that are not connected to the galaxy. The object does not appear to be undergoing any major mergers or interactions. The general appearance and structure of this galaxy are indicative of a relatively evolved system.
