The galaxy presents a generally smooth, elliptical morphology. The central region is a bright, concentrated core, suggesting a high stellar density. A faint, diffuse halo surrounds the core, gradually fading into the background. There is some evidence of redder hues in the central region, possibly indicative of an older stellar population. No distinct spiral arms or prominent dust lanes are visible. The galaxy appears largely undisturbed, with no signs of major tidal interactions or ongoing mergers. The overall color is slightly yellow-green, suggesting the presence of intermediate age stars, but this may be due to redshift.
