The galaxy presents as a somewhat elongated, cigar-shaped object. The light distribution suggests a concentration of older stars or dust in the central region, which appears more yellow/orange in color. Fainter, bluer light extends along the major axis, hinting at some degree of disk-like structure or more recent star formation activity within that plane. There's an absence of distinct spiral arms. No clear signs of a major ongoing merger are apparent, though minor irregularities or a slight disturbance cannot be completely ruled out. The overall smooth appearance leans towards an early-type or lenticular galaxy.
