The galaxy appears to be characterized by a central, bright core region indicative of a high concentration of stellar mass and possibly an active galactic nucleus. Surrounding the core is a more diffuse, extended halo, likely composed of older stellar populations. Patches of bluer light are present in what looks like a spiral arm. There is a disturbed appearance around the central core which suggests a possibility of ongoing interactions or past mergers. The overall shape of the galaxy appears somewhat distorted, not exhibiting a perfectly smooth elliptical or spiral structure. This could also indicate gravitational interaction with another galaxy, though no other companion galaxy is visible in the image.
