The galaxy appears to be a relatively compact, elliptical galaxy with a smooth, largely featureless structure. It exhibits a roughly spheroidal shape, with a slight elongation that does not suggest a significant disk component. The galaxy is primarily bluish, indicating a population of relatively young, hot stars. There's no clear evidence of spiral arms, bars, or prominent dust lanes. Minor disturbances present suggests a potential history of past mergers. The galaxy's relatively compact size suggests it is a low-mass system.
