The galaxy presents as a relatively smooth, elliptical-like structure, displaying a concentrated central bulge that transitions into a more diffuse halo. The overall color profile appears predominantly yellowish-red, suggesting an older stellar population and potentially reduced star formation activity. There is no clear evidence of spiral arms or a well-defined disk structure. The observed morphology indicates a system undergoing, or having completed, a process of morphological transformation, possibly via mergers or internal dynamical evolution. The absence of prominent tidal features or other signs of ongoing major disturbances suggests that the galaxy is relatively settled at the time of observation. The galaxy appears to be moderately massive, radiating intensely despite its red-shifted distance, indicating substantial past or present stellar luminosity.
