The galaxy appears to be a relatively compact system with a slightly elongated shape. Its core region exhibits a brighter, concentrated luminosity, possibly indicating a central bulge component. Surrounding the core, there is a diffuse, more extended disk-like structure. Within this disk, hints of spiral arm morphology might exist, though the image resolution makes it difficult to confirm definitively. The galaxy displays a color gradient, with the core and inner regions appearing more yellow/orange, suggesting an older stellar population, while the outer regions show bluer tints, potentially indicating ongoing star formation activity. A small, localized bright region is also visible. There is evidence of some slight disturbance within the galaxy, but it is difficult to determine a cause based on this image alone.
