The galaxy exhibits a generally smooth morphology with a subtle disk-like structure. Its shape appears to be somewhat elongated, leaning towards a cigar-like appearance rather than perfectly round. The central region displays a brighter luminosity, suggesting a concentration of stars or potentially an active galactic nucleus. The outer regions gradually fade into the background, lacking prominent spiral arms or distinct features. There is no major merging occurring, though there appears to be a minor disturbance. The color is consistent across the galaxy.
