The galaxy presents a generally smooth, elliptical morphology. It exhibits a concentrated central bulge, characterized by a yellowish hue, suggesting an older stellar population. A faint, diffuse halo surrounds the bulge, appearing slightly more extended along the vertical axis. Within the halo, a faint blush of red appears, indicating possible regions of on-going or recent star formation. There is no evidence of spiral arms or a well-defined disk structure. The galaxy appears relatively isolated and undisturbed, without any signs of major mergers or tidal interactions. The overall color suggests a moderate redshift and luminosity.
