The galaxy presents as a relatively smooth, elliptical-like structure with a bright, concentrated central region. The overall shape is largely round. There's a subtle color gradient visible, transitioning from a slightly redder hue in the core to a bluer halo. This may indicate an older stellar population in the central bulge and a relatively young stellar population in the outer regions. There is no apparent spiral arm structure and no evidence of significant dust lanes or tidal disturbances. The observed morphology suggests a galaxy that has undergone significant merging or secular evolution. Star formation appears to be low.
