The galaxy presents as a smooth, elongated object with a subtle color gradient. The central region exhibits a brighter, almost uniform luminosity distribution. The overall shape suggests a prolate spheroid morphology, with a significantly longer axis than its minor axis. There is no clear evidence of spiral arms, dust lanes, or active star-forming regions in the image. The color is moderately blue, suggesting a population of young stars, although the low star formation rate implies a relatively quiescent state. There appear to be no major disturbances or mergers visibly affecting its structure, although there is faint evidence of a minor disturbance.
