The galaxy exhibits a generally elongated, cigar-like morphology, with the major axis being significantly larger than the minor axis. Its light distribution appears to be relatively smooth throughout its structure, suggesting a lack of significant spiral arms or other prominent features. There is a central concentration of light, appearing as a slightly brighter region within the galaxy, perhaps indicating the presence of a bulge. The overall color of the galaxy is somewhat blue, hinting at a population of young, hot stars, and ongoing star formation, albeit potentially at a low rate. There is no obvious visual evidence of any ongoing major mergers or significant tidal disturbances within the galaxy's structure; it appears to be relatively isolated and undisturbed.
