The galaxy presents as a relatively smooth, elongated object. Its light distribution appears largely uniform, lacking prominent spiral arms or a distinct bulge. The overall morphology suggests a disk galaxy viewed at a high inclination. Color gradients are subtle, with a slightly bluer hue towards the edges compared to the central region. The galaxy exhibits a small scale length, appearing compact in size. There are no indications of major mergers or significant tidal disturbances in the immediate vicinity, but there may be faint light extending beyond the primary body of the galaxy, suggesting a possible minor interaction in the past. It appears to have a low star formation rate.
