The galaxy presents as a slightly inclined spiral type. Relatively well-defined spiral arms appear to emanate from a central bulge region. The spiral arms show a granular texture, indicative of active star formation. The color of the arms tends towards blue, which implies a population of hot, young stars, consistent with the presence of star formation regions. The bulge exhibits a less pronounced color contrast. There appears to be a possible bar structure with a moderate presence. The disk is not viewed perfectly edge-on, with an estimated tilt that allows some spiral arm structure to be visible. Overall, the galaxy appears relatively isolated, showing no signs of major disturbances or ongoing mergers.
