The galaxy presents as an elongated, cigar-shaped structure. The light distribution is mostly smooth, with a concentrated central bulge displaying a yellowish-orange hue, indicative of older stellar populations. Fainter, bluer light extends along the major axis of the galaxy, possibly indicating the presence of more recent star formation. There appear to be some minor disturbances or irregularities in its overall form, but these do not suggest an ongoing major merger event. The galaxy appears relatively isolated, with no other nearby galaxies visibly interacting with it.
