The galaxy presents as a single, centrally concentrated light source with a relatively smooth morphology. It appears to be primarily spheroid-shaped, exhibiting minimal evidence of spiral arms or significant structural features. There may be a small hint of a disk-like feature. The central region is noticeably brighter, indicating a concentration of stars and potentially a supermassive black hole. The overall color is yellowish, suggesting a population of older stars, and lower amounts of ongoing star formation. No signs of tidal tails or significant interactions with other galaxies are visible. There is little to no evidence of dust lanes or patchy star formation regions.
