This galaxy presents a morphology that appears to be characterized by both smooth and featured components. The central region exhibits a concentrated luminosity profile, potentially indicating the presence of a significant bulge component. A disk-like structure is also visible, with hints of spiral arm formations extending outwards from the central bulge. These spiral arms appear somewhat flocculent and ill-defined, exhibiting a patchy distribution of star formation regions.

The color distribution suggests active star formation is occurring. The outer regions of the galaxy appear bluer, suggesting a population of younger, hotter stars. The central region exhibits yellower colors, perhaps indicative of an older stellar population or dust obscuration.

There is also evidence of potential interactions. The overall shape of the galaxy appears somewhat disturbed, with asymmetries in the distribution of light. This could indicate recent or ongoing mergers or tidal interactions with another galaxy.
