The galaxy presents as a diffuse, elliptical-shaped object with a concentrated central region. The core exhibits a bright, yellowish hue, indicative of an older stellar population. Progressing outwards from the core, the light intensity decreases gradually. There is minimal indication of distinct spiral arm structures or dust lanes within the galaxy's morphology. The overall smooth appearance suggests a relatively relaxed system. Subtle deviations from perfect ellipticity may be present, hinting at possible minor interactions or internal kinematic disturbances. However, the lack of strong tidal features suggests that if any interaction is present, it is not in an advanced state of merging.
