The galaxy presents as a relatively small, elongated structure with a noticeable disk. It exhibits a smooth, yet slightly disturbed morphology, hinting at possible past or ongoing interactions. The color distribution suggests a population of older stars, with a redder hue dominating the galaxy's overall appearance. A faint disk is visible, with the suggestion of spiral arms or features within it. There is no distinct central bulge that can be obviously seen. The galaxy shows no distinct signs of a major merger, but there is a slight asymmetry.
