The object presents as a single, fairly symmetrical galaxy. Its overall morphology appears largely smooth, with a central concentration of light suggestive of a prominent galactic bulge. The color profile is predominantly red, with a noticeable concentration of redder light towards the core region. This may indicate an older stellar population dominating the galaxy, particularly in the central bulge. A faint, diffuse halo surrounds the central region, extending outwards with a gradual decrease in surface brightness. There are hints of some minor disturbances or irregularities in the outer regions. The data suggests a considerable stellar mass. The galaxy appears to be undergoing low levels of star formation. Overall, it seems likely that this is a massive, relatively evolved galaxy with ongoing, albeit limited, star formation activity.
