The galaxy presents an elongated, cigar-shaped morphology. Its light profile appears relatively smooth, lacking prominent spiral arm structures or strong indications of dust lanes. The color gradient suggests a possible red sequence galaxy, with a yellowish-orange hue indicative of an older stellar population, though a small component of bluer light exists. There is no evidence of a major merger event. Minor disturbances cannot be entirely ruled out but do not obviously disrupt its structure. Overall, the galaxy appears as a relatively undisturbed elliptical or lenticular galaxy.
