The galaxy presents as a lenticular, cigar-shaped form, appearing elongated along its major axis. The bulge is not particularly prominent, appearing somewhat flattened. There is a distinct disk component visible; however, the spiral arms are not well-defined. Color gradients are subtle, with a slightly bluer hue visible in regions within the disk, suggesting ongoing, though perhaps modest, star formation. The smoothness of the overall light distribution is moderately high. There is no clear evidence of a major ongoing merger, although there may be slight disturbances indicative of minor interactions. The angular size is small.
