The galaxy presents a largely smooth morphology, with a concentrated central bulge. It exhibits a roughly elliptical shape, showing no prominent spiral arm structure. The light distribution is generally even, with a gradual falloff in intensity from the core. Color gradients suggest a higher concentration of older stellar populations in the central regions, trending towards slightly bluer hues in the outer regions, though star formation appears subdued. The overall structure does not show any signs of significant tidal disturbances or ongoing major merger events.
