The galaxy presents an elongated, cigar-shaped morphology. Its light distribution is concentrated toward the center, with a yellowish core suggesting an older stellar population. Fainter extensions of light are visible along the major axis, appearing more reddish, possibly indicating dust lanes or regions of ongoing star formation. There seems to be an absence of clearly defined spiral arm structures in the image. The galaxy appears relatively smooth overall, with a lack of clumpy or irregular features. Its estimated size is roughly 5.4 kpc, and it is currently receding away from us at roughly 13% the speed of light.

