The observed galaxy presents a lenticular morphology, viewed at an almost edge-on inclination relative to our line of sight. The central bulge appears relatively small, indistinct and smooth, suggesting an older stellar population. A flattened disk component is clearly visible, exhibiting a radial color gradient. The color transitions from a bluer hue at the edges towards redder colors in the central region of the disk. This may suggest that the star formation rate is higher at the edges of the disk, and lower towards the center of the disk. There is no visible evidence of strong spiral arm structure or prominent dust lanes, although this could be obscured by the inclination. The galaxy is likely in a relatively quiescent state, with no major ongoing mergers or interactions evident.
