The galaxy exhibits a disturbed morphology, indicating a potential interaction or merger. The central region displays a concentrated luminosity with a yellowish hue, potentially indicating an older stellar population. Extended from this core, there appears to be a diffuse blue halo or tidal feature, indicative of ongoing or recent star formation activity. The overall shape is irregular, deviating significantly from a classic elliptical or spiral structure. There is a significant amount of blue light indicating this galaxy is likely in its blue cloud phase of evolution. The substantial blurring suggests the galaxy is relatively distant. Patches of slightly brighter emission are noted towards the outer edges of the galaxy, indicating potentially some HII regions. 
