The galaxy presents an elongated, cigar-like morphology. It exhibits a smooth, featureless appearance with a central bulge that appears brighter and more concentrated than the outer regions. The galaxy's color gradient suggests an older stellar population, with a yellowish-red hue dominating the light emitted. No distinct spiral arms or dust lanes are discernible in the image. The absence of prominent star-forming regions and its shape hint at a possible elliptical classification, with a high probability that it has no major mergers occurring. Overall, it appears to be a relatively quiescent system.
