This galaxy presents as a relatively small, elongated object with a noticeable central bulge that is brighter and appears somewhat spherical. Faint spiral arms or extended features are suggested, emerging from the core, with what looks like dust lane features trailing away from the main body of the galaxy. The light profile appears to decrease gradually from the center outwards. The color is bluish, indicating possibly younger, hotter stellar populations, with some regions being more blue than others. There may be some minor distortions visible in the disk suggestive of past interactions, with the faint extended features potentially influenced by tidal forces. Further spectral analysis would be necessary to confirm star formation rates and galactic composition.
