The galaxy presents as a relatively compact object. The central region appears bright and unresolved, suggesting a dense concentration of stars. The overall morphology is somewhat smooth, with no prominent spiral arms or bar structures easily discernible. 

A faint, diffuse halo surrounds the bright core, exhibiting a subtle color gradient. The inner halo appears slightly bluer than the outer regions, potentially indicating younger stellar populations closer to the galactic center. There might be some minor asymmetry or disturbance in the outer halo, which may be indicative of a weak tidal interaction. The galaxy displays a minor irregularity to the upper right, which may be a sign of a past or ongoing minor merger event.
