The galaxy presents as a relatively compact object. Its morphology appears complex, showing characteristics that suggest possible interaction or disturbance. At its core, a bright, concentrated region dominates, indicative of a high density of stars or active galactic nucleus activity. Surrounding this central region is a less defined, asymmetrical structure. There are faint extensions or tidal features that may be indicative of gravitational interactions. Color variations are subtle, with a generally blue hue, potentially indicating the presence of younger stars or regions of active star formation. The overall impression is of a galaxy that is either actively merging with another or has experienced a recent gravitational disturbance.
