This galaxy exhibits a smooth, elongated morphology, appearing cigar-shaped in its overall form. The light distribution suggests a relatively uniform stellar population, with a gradual increase in brightness towards the central region. The lack of distinct spiral arms or prominent dust lanes indicates a relatively quiescent galaxy, potentially an elliptical or lenticular type. The blue hue suggests that there may be some recent star formation activity, however, this is limited. Based on the color, this galaxy is likely an older galaxy with an estimated stellar mass of 10^9.4 solar masses. There is no significant evidence of tidal disturbances or mergers in this image.
