The galaxy presents a generally smooth appearance, with an elongated, cigar-like morphology. It exhibits a luminous central bulge that dominates the light output. To one side, there is a fainter, bluer extension that may indicate the presence of a galactic disk component. The smooth appearance suggests a relatively evolved system, though some minor disturbances cannot be ruled out. The color gradient, from the redder bulge to the bluer extension, implies ongoing star formation in the disk. The size is consistent with a typical dwarf galaxy. Overall, this appears to be a late-type galaxy with a prominent bulge and hints of a spiral structure.
