The galaxy presents as a lenticular or possibly an elliptical galaxy, elongated in shape. Its central bulge appears relatively smooth and concentrated, exhibiting a yellowish-white hue, indicative of an older stellar population. A faint disk-like structure extends outward from the bulge, with hints of spiral arms. There appears to be a moderate amount of dust and gas present within the disk, observable by slightly green features. The galaxy shows little evidence of recent or ongoing major mergers, though there is a minor asymmetry that could be related to a past interaction. The overall appearance suggests a galaxy in a transitional phase, potentially evolving from a spiral to a lenticular morphology, having exhausted most of its gas reservoir for star formation.
