The galaxy presents a generally smooth and rounded appearance. It displays a concentrated central bulge of yellowish hue, suggesting an older stellar population. Surrounding this core is a more diffuse and slightly bluer halo, indicative of ongoing or recent star formation activity. There is no discernible spiral structure or distinct disk component; rather, it exhibits a lenticular-like morphology. Faint hints of asymmetrical light distribution within the outer regions suggest the possibility of minor gravitational interactions, although no clear signs of tidal tails or ongoing merger events are observed. The galaxy appears to be relatively isolated, which aligns with the smooth features displayed. The bluer, more diffuse outer regions and the yellow center suggest it may be transitioning away from vigorous star formation towards a redder, quiescent state.
