The galaxy presents as a fairly smooth, rounded structure with a concentrated central bulge. There is little evidence of distinct spiral arms or a prominent disk. The primary color is a yellowish-white, suggesting an older stellar population, with potentially less active star formation. Subtle color variations exist within the galaxy's extent; the central region appears more yellow than the surrounding halo, suggesting a higher concentration of older, redder stars there. Overall, the galaxy exhibits a morphology consistent with an elliptical or lenticular type. There is no evidence of any ongoing major merger events, although some minor disturbances or tidal features cannot be completely ruled out given the image resolution.
