This galaxy appears to be a relatively smooth, disk-shaped system, observed at an oblique angle. A central bulge is evident, exhibiting a yellowish-orange hue, potentially indicative of an older stellar population. Surrounding the bulge is a fainter disk, appearing somewhat elongated and diffuse. Hints of bluer regions can be discerned within the outer disk, suggesting areas of more recent star formation, although these are not highly pronounced. There is no readily apparent spiral structure or prominent dust lanes. The galaxy does not show any indications of major mergers or significant tidal disturbances, but subtle irregularities in the outer regions cannot be ruled out. Overall, the galaxy presents as a moderately luminous, disk-dominated system with signs of ongoing, but subdued, star formation.
