The galaxy presents as a somewhat elongated, disk-like structure. A central bulge is apparent, exhibiting a bright, concentrated luminosity, indicative of a high stellar density. Moving outwards from the core, the galaxy appears to transition into a less structured disk. The disk demonstrates a color gradient, shifting from yellow towards slightly redder hues. There are some indications of possible faint spiral arm structure, however, the image resolution makes this difficult to confirm definitively. The overall appearance suggests a relatively evolved system, but shows minor disturbances, possibly an ongoing or recent interaction.
