The galaxy presents as a centrally concentrated object with a slight elongation. A distinct bulge is apparent, transitioning smoothly into a disk component that appears relatively featureless. The overall color gradient suggests a higher concentration of older stellar populations in the bulge, shifting towards younger, bluer stars in the outer regions. There may be minor irregularities in the outer disk, however the resolution is too low to assess if there are any disturbances, merging activity, or evidence of spiral arm structure. The galaxy exhibits a relatively high degree of central symmetry.