This galaxy presents as a somewhat flattened spheroid with a bright, concentrated central bulge. The light distribution indicates a smooth profile, with a distinct lack of prominent spiral arms or other strong morphological features typically associated with late-type spiral galaxies. There is evidence of a disk component, seen as a slight flattening and subtle extension along a preferred axis.

The color gradient suggests an older stellar population, particularly within the central bulge, as indicated by the yellow-orange hue. Fainter blue hints at a more modest recent star formation activity within the surrounding disk, albeit not at a rate high enough to give it a strong blue color. 

There may be a minor disturbance present, but it is likely the galaxy has not undergone any major mergers recently.
