The galaxy presents as a relatively smooth, elongated structure. Its overall shape appears to be somewhat cigar-shaped. There is a subtle color gradient present, with a central region exhibiting a warmer hue, possibly indicative of older stellar populations. Fainter, cooler tones surround this central region, with an apparent lack of distinct features like prominent spiral arms or concentrated star-forming regions. There may be a slight disturbance in the light profile of the galaxy indicating an ongoing or previous minor disturbance.
