The galaxy presents as a relatively smooth, elongated structure. Its overall shape is somewhat cigar-shaped, with the central region appearing brighter and more concentrated than the outer edges. The color appears to be a soft, bluish-white, suggesting the presence of a population of relatively young, hot stars. There is no obvious spiral structure or distinct disk features visible. No significant signs of on-going major merger activity are apparent. The slight elongation may indicate a minor disturbance or ongoing tidal interaction, but overall, the galaxy presents as a settled system.
