The galaxy presents as a relatively small, cigar-shaped system. Its overall light distribution appears smooth, lacking prominent spiral arm structures or a distinct bulge. The color profile suggests a higher concentration of blue light towards the central region of the disk, which may indicate ongoing star formation. The galaxy does not show signs of major mergers, though there might be very subtle signs of minor gravitational disturbance. Given its elongated shape, it could be classified as a lenticular galaxy, viewed nearly edge-on.
