The galaxy presents as a relatively compact object with a bright central region. The core exhibits a high surface brightness, appearing almost unresolved in this image. Extending outward from this core, there is a diffuse, disk-like structure. The color distribution suggests a radial gradient, with bluer tones concentrated in the central regions and a shift toward redder hues in the outer parts of the disk. There is a slight asymmetry in the galaxy's structure, possibly hinting at a minor interaction or disturbance. Definite spiral arms are not visible, with the object appearing to be on the smoother end of the spectrum. The central concentration dominates the overall light profile. There is a possible indication of tidal features near the central mass.