The galaxy presents as a relatively smooth, disk-like structure with a slightly elongated, cigar-shaped morphology. A pronounced central bulge is observed, exhibiting a yellowish hue, indicative of an older stellar population and potentially lower levels of ongoing star formation. The outer regions of the galaxy display a bluer color, suggesting the presence of younger, hotter stars. There is a subtle indication of faint spiral arm structure, though not prominently defined. No signs of significant tidal disturbances or ongoing mergers are immediately apparent. The overall appearance suggests a galaxy that is well-evolved, and relatively undisturbed.
