The galaxy presents as a relatively smooth, elongated structure. Its overall color appears to be a subdued bluish-white, suggesting a moderate population of young, hot stars. The light distribution is fairly uniform across the visible body, indicative of a well-mixed stellar population. No prominent spiral arms or dust lanes are discernible in the image. The galaxy exhibits a slight cigar shape, with an axis ratio that deviates noticeably from unity. There is no evidence of a prominent nucleus or central bulge. The outer edges are somewhat ill-defined, blending gradually into the background sky. There is no noticeable interaction with any other galactic bodies or other disturbances. 
