The galaxy exhibits a slightly irregular morphology. At its core, a bright, concentrated region is observed, appearing almost stellar in nature. Surrounding this central region is a less defined halo of diffuse light. The color distribution suggests varying stellar populations or dust content within the galaxy. A distinct green hue is visible in the outer regions, possibly indicative of ongoing star formation or emission from ionized gas. Patches of blue are also observed, potentially indicating the presence of younger, hotter stars. The overall structure appears somewhat disturbed, potentially due to a past or ongoing interaction with another galaxy, though no obvious merging partner is immediately apparent. There is some indication of possible tidal features, though they are faint and not clearly defined.
