The galaxy presents as a somewhat amorphous, though generally rounded structure, with a relatively smooth light distribution. Its central region appears more luminous and concentrated compared to its outer edges. Faint, asymmetric extensions or tidal features are potentially present, suggesting possible past or ongoing gravitational interactions. There may be a recent or ongoing minor merger that is causing this. Color gradients are observed within the galaxy, transitioning from more bluish hues in the outer regions to reddish hues in the inner regions. This suggests the possibility of differential stellar populations and star formation activity within the galaxy, with younger, hotter stars potentially dominating the outer regions and older, cooler stars concentrated in the central bulge. The overall appearance could be consistent with an early-type galaxy exhibiting signs of disturbance or recent accretion. There appear to be some clumps of stars or star clusters embedded within the galaxy's halo, suggesting the possibility of star formation or accreting galaxies.
