The galaxy presents as a relatively small, lenticular or early-type spiral galaxy. It exhibits a smooth, centrally concentrated bulge that dominates the overall light profile. The bulge appears nearly spherical. There is evidence of a faint, flattened disk component surrounding the bulge. The galaxy is positioned at an angle relative to our line of sight, appearing nearly edge-on, although subtle disk features suggest a slight inclination. The color profile indicates a population dominated by older stars, with a general lack of prominent blue star-forming regions. The morphology suggests the system is relatively undisturbed with no signs of major ongoing mergers or tidal distortions. Minor irregularities may be present within the disk, though they are difficult to resolve due to the galaxy's distance and relatively small angular size.
