The observed galaxy exhibits an overall elliptical morphology, appearing flattened along its major axis. The central region displays a concentrated, bright core, suggestive of a significant stellar population and/or an active galactic nucleus. A faint, disk-like structure is visible, oriented edge-on relative to our line of sight. The galaxy's color profile indicates a bluer hue in the outer regions, potentially indicative of younger stars or ongoing star formation. Subtle indications of a minor disturbance or tidal feature may be present in the outer halo region, though the signal is weak. Overall the galaxy looks like an elliptical with a disk.
