The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated core. The light profile appears to decrease gradually from the center outwards, lacking distinct spiral arms or prominent features usually associated with disk galaxies. There is little indication of ongoing major mergers, though some faint irregular structures around the edges could indicate minor tidal disturbances or interactions. The overall color seems to be leaning towards the redder end of the spectrum, suggesting an older stellar population. Its round shape and the overall smoothness of the light distribution hint at a relatively evolved system, possibly an elliptical or lenticular galaxy type. Star formation appears to be low.
