The galaxy presents a relatively compact appearance. Its overall structure suggests a transition between smooth and disk-like morphology. While some regions exhibit a diffuse, amorphous quality, there are hints of a more structured organization. There is a central bright bulge surrounded by a fainter, more extended disk.

The color profile appears to be multi-hued, with a bluer core region, transitioning to redder colors towards the outer edges. This could be indicative of ongoing star formation in the central bulge. There are indications of minor disturbances in the overall shape, potentially suggestive of gravitational interactions or tidal effects from past or ongoing merger events. However, there is no clear evidence of major disturbances to the galaxy's morphology.
