This galaxy appears to be a relatively face-on spiral galaxy, exhibiting a prominent central bulge. The bulge displays a yellowish hue, suggesting an older stellar population dominated by evolved stars. The surrounding disk shows evidence of spiral arm structure, albeit somewhat flocculent and not tightly wound. These arms have a bluer coloration indicative of ongoing star formation and the presence of younger, hotter stars.

The overall morphology leans towards a disk-dominated system, with the bulge contributing significantly to the galaxy's luminosity. There is no immediately obvious sign of strong tidal disturbances or interactions, suggesting it is a relatively isolated system. The surface brightness is moderately high, indicating a substantial stellar density, particularly towards the central regions.
