The galaxy presents as a centrally concentrated object, appearing relatively smooth in morphology. Its light profile seems mostly uniform, without prominent spiral arms or a distinct bar structure. The galaxy exhibits a predominantly blue hue, suggesting the presence of relatively young, hot stars and active star formation. The overall roundness suggests a possible elliptical or S0 morphology, rather than a late-type spiral, though some disk features could be present. There is slight asymmetry, possibly from a minor gravitational disturbance. No obvious signs of tidal tails or merging features are evident. 
