The observed galaxy presents as an elongated, disk-like structure, viewed at a nearly edge-on inclination. There is a pronounced central bulge region that appears bright and somewhat diffuse. The color of the bulge is generally yellowish. Fainter, bluer light emanates from the outer regions of the disk suggesting possible star formation. Dust lanes may be present, but are difficult to discern. There are no distinct spiral arms visible, likely due to the high inclination. The galaxy exhibits a generally smooth appearance, with some possible minor disturbances in the outer disk. The overall structure does not suggest any significant ongoing merger activity. The size of the galaxy is relatively small.
