The galaxy exhibits a distinct elongated, cigar-like morphology. It appears as a relatively smooth structure, though with some indication of features or a disk-like component. A blue hue is noticeable, suggestive of ongoing star formation. There is no obvious evidence of a major merger or significant disturbance in its structure. It appears to be a relatively low-mass system, with modest star formation activity. The galaxy's half-light radius is estimated to be several kiloparsecs.
