The galaxy presents as a moderately bright, somewhat elongated object with a relatively smooth and concentrated central bulge. It appears to be disc-dominated, but the disc component is not highly structured; there is a notable absence of prominent spiral arms or distinct dust lanes. The colour appears to be subtly bluer in the outer regions of the disc, perhaps indicative of younger stellar populations or ongoing star formation there. The overall shape is not perfectly circular, exhibiting a mild cigar-like morphology, suggesting a possible triaxial structure or the result of a minor interaction. There is no strong evidence of a major merger or significant tidal disturbance in the immediate vicinity.
