The galaxy presents a somewhat elongated, cigar-shaped morphology. It exhibits a smooth, relatively featureless appearance, with a gradual decline in surface brightness from the central region outwards. The light distribution suggests a predominantly elliptical shape. A slight asymmetry is visible, perhaps due to a minor gravitational interaction or internal dynamics. The color appears bluish, particularly towards the central region, which is consistent with the presence of younger, hotter stars. The relatively compact size suggests it could be either a dwarf galaxy or a more distant, larger system. Star formation is ongoing, but at a relatively low rate. The galaxy does not show any strong evidence of a major merger event, although some minor disturbances cannot be ruled out.
