The galaxy appears to be an elliptical type, exhibiting a smooth, concentrated light profile. The central region displays a bright, yellowish-white color, indicating a significant population of older stars. There is a slight elongation in the overall shape. The faint, diffuse blue light extending outward suggests ongoing, but low level, star formation activity in its outer regions. The object is likely a massive galaxy, undergoing some interaction that may be the cause of the extended star formation. There may be an active galactic nucleus (AGN) based on the very bright core.
