The galaxy presents an irregular morphology. There appears to be a central, somewhat brighter region with a slight elongation. This core exhibits a color gradient, transitioning from a more reddish hue on one side to a bluer tint on the opposite.  A fainter, diffuse extension is visible, suggestive of a tidal tail or disrupted structure, indicating possible past or ongoing interaction with another galaxy. The overall color of the galaxy is largely composed of redder wavelengths, implying an older stellar population with potentially suppressed star formation.  There are areas which are more blue in color, so star forming regions are potentially present.  The overall appearance suggest the system has experienced gravitational disturbances, possibly related to a merging event.
