The galaxy presents an elongated morphology, appearing cigar-shaped. A smooth central bulge is evident, exhibiting a bright, concentrated luminosity. Extending from this central region is what appears to be a tail, possibly a tidal tail, or an extended feature caused by galactic interaction. This "tail" shows a color gradient, transitioning from yellow-orange near the center to a faint blue at its extremity, indicative of a potential difference in stellar populations. The central bulge appears largely featureless, and the galaxy is non-merging. Faint disturbances may be present within the tail-like feature.