The galaxy presents as a smooth, elongated structure. It displays a dominant central bulge, which appears yellow-orange in color, indicating a likely older stellar population. The outer regions of the galaxy show a gradual decline in surface brightness. These outer regions display a bluer hue. This suggests the presence of a younger, star-forming stellar population. The overall shape is cigar-like, with no apparent spiral arm structure or significant dust lanes visible in the available image resolution. There are no clear signs of major mergers or significant tidal disturbances. However, subtle distortions are possible within the noise level. The luminosity profile suggests a relatively concentrated mass distribution.
