The galaxy presents a somewhat elliptical morphology. It possesses a bright, concentrated central region, potentially indicative of an active galactic nucleus or a dense stellar population. The overall color appears to be a mix of blue and red, with the central region exhibiting a whiter hue, which suggests a range of stellar ages within the galaxy. Fainter, less distinct arm-like structures or irregular features are visible extending outwards from the central region. A minor degree of disturbance is apparent in the galaxy's shape, suggesting possible past interactions or mergers. There is no obvious strong ongoing star formation within the galaxy. 
