The galaxy presents a mostly smooth appearance, but there are some notable features. The overall shape appears somewhat elongated, possibly cigar-shaped, although the image resolution limits precise morphological classification. There is a brighter central region which likely corresponds to the galactic bulge. Fainter, diffuse light extends outwards from the center, suggesting the presence of a disk or more extended stellar halo. There is potential visual evidence of a merger or interaction, with a possible disturbance in the light distribution on one side of the galaxy. The galaxy's color is generally blueish, which would likely correlate with younger stars and ongoing star formation. The estimated size indicates a dwarf galaxy, and, coupled with the noted star formation, implies a lower mass system. There does not appear to be a strong spiral structure, although, again, resolution is a limiting factor.
