The observed galaxy presents as a lenticular or early-type spiral galaxy, viewed at an oblique angle. The galaxy exhibits a bright, concentrated central bulge, surrounded by a flattened disk component. There's a slight elongation in the galactic structure, with a discernible major axis. The disk appears relatively smooth, hinting at either a lack of prominent spiral arms or a highly flocculent spiral structure not easily resolved in the image. The color profile shows a yellow-white hue towards the center, gradually shifting to a bluer tint towards the outer disk. This may indicate an older stellar population concentrated in the bulge, with younger, bluer stars distributed within the disk. There may be evidence of dust or star formation, giving the outer region of the disk a light blue hue. 
