The galaxy presents as a largely featureless, smooth object with a somewhat round morphology. There may be a slight elongation along one axis, but the overall shape approximates circularity. A central, bright region is observed, possibly indicative of a concentrated galactic nucleus. Fainter, diffuse light extends outwards from this central area, suggesting a surrounding halo or disk component. Overall color appears slightly blueish white, hinting at a population of younger, hotter stars, potentially with ongoing, low levels of star formation. There is no obvious evidence of spiral arm structure or major disturbances. The galaxy appears to be relatively isolated, without any clear signs of interaction or merging activity.
