This galaxy appears to be a relatively compact object. It exhibits a somewhat irregular morphology. There is a suggestion of some tidal disruption or interaction with another galaxy, although the disturbances appear minor. The galaxy presents a faint and diffuse halo or envelope extending beyond its brighter central region. The color indices suggest that there may be a complex mix of stellar populations, with the central region exhibiting a somewhat bluer color than the outer regions, which appear redder. The blue color indicates younger, hotter stars while the redder colors suggests a population of older, cooler stars. Overall, this galaxy seems to be a system undergoing some kind of minor interaction or disturbance, possibly a past minor merger. 
