The galaxy presents as a fairly smooth, elliptical or lenticular type, with a high degree of central concentration. The overall color is a yellowish-orange, suggesting a dominant population of older stars. There is some subtle color variation across the galaxy; the central bulge appears more orange, while the outer regions exhibit a slightly bluer hue. This might indicate a small amount of ongoing star formation in the outer parts of the galaxy, though it is not pronounced. The galaxy is elongated, with an apparent axis ratio suggesting it is viewed at a moderate inclination. No distinct spiral arms or other prominent features are discernible. The overall impression is of a mature galaxy with a well-established stellar population. There appears to be little sign of major recent merger activity or significant disturbances in its structure.
