The galaxy presents as a somewhat elongated, lenticular structure. A bright, concentrated central bulge dominates the galaxy's morphology, exhibiting a yellow-orange hue, potentially indicating an older stellar population. A fainter, diffuse disk surrounds the bulge. The disk shows hints of blue-ish tones which may suggest regions of more active star formation, although the disk appears relatively smooth and featureless, lacking prominent spiral arms. The overall color gradient suggests a transition from older stars in the bulge to potentially younger stars in the disk. The galaxy does not appear to be undergoing any major merging events or significant tidal disturbances. It's possible minor interactions may be occurring given the slight asymmetry of the outer disk, but this is not conclusive from the image alone. The galaxy appears to be relatively isolated in its environment.
