The galaxy presents as an elongated, somewhat cigar-shaped structure. Its light is dominated by a blue hue, indicating a population of younger, hotter stars. The central region exhibits a brighter, more concentrated glow, suggesting a higher stellar density within the core. There appears to be some distortion, and perhaps a very minor interaction may be occurring. However, the overall shape is relatively undisturbed. The galaxy appears to be undergoing moderate levels of star formation but is generally not very luminous overall.
