The galaxy presents as a relatively smooth, lenticular or early-type spiral galaxy, exhibiting a notable lack of distinct spiral arm structure. Its overall form is elliptical. The central bulge region appears bright and concentrated, with a fairly uniform intensity, suggesting an older stellar population. Moving outward from the bulge, the galaxy exhibits a gradual decrease in luminosity. The disk component is faintly visible. There are subtle color variations, with a slightly bluer hue in the outer regions of the disk, possibly indicating regions of ongoing or recent star formation, while the central bulge is a more yellow color. There is no evidence of a significant tidal disturbance. Based on these characteristics, the galaxy appears to be relatively evolved and isolated.
