The galaxy presents as a mostly smooth, lenticular structure, approximately elliptical in shape, though with some deviation. The central bulge appears bright and exhibits a reddish-yellow hue, indicating an older stellar population. The disk component surrounding the bulge displays a greener tint, suggesting the presence of younger stars and possibly ongoing star formation, albeit at a relatively low rate. There is faint evidence of a possible disturbance or minor interaction within the disk. No strong spiral arms are discernible. The galaxy displays a round morphology, with only slight elongation. Based on the observed characteristics, this galaxy is likely to be a transitioning system between a spiral and an elliptical galaxy, dominated by an evolved stellar population in the bulge and a moderately active disk.
