The galaxy presents as a face-on spiral, exhibiting a distinct central bulge surrounded by a flattened disk. Two spiral arms emanate prominently from the central region. These arms are tightly wound near the center, gradually loosening as they extend outwards. The luminosity distribution within the galaxy shows a strong concentration towards the core, indicating a relatively old stellar population within the bulge. The disk displays a bluer hue compared to the bulge, suggesting the presence of younger, hotter stars and ongoing star formation within the spiral arms. There is no evidence of significant tidal disturbances or ongoing merger activity; however, there appears to be a slight asymmetry in the outer regions of the disk, hinting at a possible past interaction or subtle internal dynamics. The galaxy appears relatively undisturbed.
