The galaxy appears to be a relatively compact, luminous object. It exhibits a concentrated central region, possibly a bulge, that dominates the overall light profile. Surrounding this central area is a more diffuse halo or extended disk component. The disk shows signs of possible minor irregularities or distortions, although the resolution limits definitive morphological classification based on features. The overall color profile suggests a mix of stellar populations, with the central region perhaps skewed slightly towards older, redder stars, while the surrounding disk may harbor younger, bluer populations. There is some indication of low-level disturbances or interactions, however it is ambiguous.