This galaxy appears to be a relatively smooth, elliptical-like structure with a bright central core. There is a noticeable lack of distinct spiral arm features or significant dust lanes. The overall shape is generally rounded, though it deviates slightly from perfect circularity. The light distribution suggests a concentration of stars and possibly a supermassive black hole within the galactic center. There appears to be some minor visual disturbance on the edge of the galaxy, but it is not obviously experiencing an active merger or major tidal disruption. The galaxy's color is indicative of an older stellar population with a lack of new star formation. A smaller secondary object is potentially gravitationally interacting with the main galaxy.
