The galaxy presents an elongated, cigar-shaped morphology. It appears relatively smooth in structure, exhibiting a soft, diffuse glow with no distinct spiral arms or prominent features. Color gradients suggest a possible redder core, with slightly bluer hues on the outer edges. Given the lack of apparent dust lanes or active star-forming regions in the image, the galaxy likely has a relatively low star formation rate and is comprised primarily of older stellar populations. There is no evidence of a recent or ongoing major merger event.
