The galaxy presents as a fairly smooth, elliptical-like structure with a dominant, concentrated central bulge. There is a noticeable decrease in luminosity moving from the core outwards, suggesting a lack of significant ongoing star formation in the outer regions. The overall color appears to be slightly yellow/red, implying an older stellar population. There is no clear evidence of a disk structure or spiral arms. The galaxy exhibits a degree of roundness in its shape and does not show obvious signs of recent or ongoing major merger activity. There is only minor asymmetry or disturbance.
