This galaxy presents a generally smooth and concentrated morphology. The central bulge appears significant, exhibiting a relatively high surface brightness and a yellowish-orange hue, suggesting an older stellar population. The galaxy appears somewhat elliptical in shape, more leaning towards being in between round and cigar shaped than perfectly round. Faint extensions of light are visible beyond the central region, implying the presence of a disk, though the low resolution makes it difficult to ascertain distinct spiral structures or star-forming regions within it. There is no obvious sign of any other merger or disturbance, minor or major.