The galaxy exhibits a somewhat elongated, cigar-like morphology. It appears relatively smooth, with a dominant central concentration of light. The color profile suggests a population of older stars, with a bluer region potentially indicating some ongoing or recent star formation. There may be some minor disturbances within the galaxy's structure, hinting at a possible interaction or past merger event, but the overall structure seems largely undisturbed. No prominent spiral arms or strong dust lanes are discernible in this image. The galaxy appears relatively compact.
