The galaxy presents a smooth, elliptical morphology, elongated along its major axis. The central region exhibits a concentrated, bright core, possibly indicating the presence of a supermassive black hole or a dense concentration of older stars. There is a gradual decrease in luminosity from the center outwards, with no distinct spiral arms or prominent dust lanes visible. The color profile suggests a population of older stars, as evidenced by the reddish-orange hue. There is a faint, bluish tinge around the outer edges, which may indicate a small amount of ongoing star formation in these regions. Overall, the galaxy appears to be relatively undisturbed, with no significant signs of recent mergers or tidal interactions. The galaxy measures approximately 8.6 kpc across. The galaxy exhibits an estimated redshift of 0.229, indicating its considerable distance.
