The galaxy presents as an elliptical morphology, exhibiting a smooth, relatively featureless structure. It has a notable elongation, appearing cigar-shaped with a high degree of oblateness. The central region shows a concentration of light, suggesting a prominent galactic bulge. A smooth gradient of light decreases outwards from the core, fading into the background sky. There appears to be no clear evidence of spiral arms or significant dust lanes, although faint, subtle colour variations suggest underlying structures and a low level of on-going star formation. No tidal tails or other merger-related morphological disturbances are clearly visible.
