The galaxy presents an elliptical morphology, appearing largely smooth with no readily discernible spiral arm structure. It exhibits a concentrated central bulge that appears bright yellow. Moving outward from the center, there is a gradual decrease in luminosity. The disk appears to be oriented with its major axis elongated horizontally across the image. The color of the disk shifts towards redder hues in the outer regions of the galaxy, suggesting an older stellar population with less ongoing star formation. There is no evidence of a major merger, although some subtle asymmetries in the outer regions could indicate minor tidal disturbances. The overall structure is relatively regular with a clear, smooth profile.
