The galaxy presents as an elongated, cigar-shaped structure with a concentrated central bulge exhibiting a yellowish hue, suggesting an older stellar population. The outer regions of the galaxy appear fainter and bluer, possibly indicating areas of more recent, albeit subdued, star formation. The overall form appears relatively smooth, lacking prominent spiral arms or significant dust lanes, with a disk component that is significantly inclined relative to our line of sight. The ellipticity is quite pronounced, as seen by the high ratio of the major and minor axes. There are no obvious signs of active galactic nuclei activity or ongoing major mergers, although some minor distortions within the galaxy's structure cannot be completely ruled out from this imagery.
