The galaxy presents as a smooth, elongated structure. The color is a somewhat muted blue, concentrated towards the center of the galaxy, suggesting a population of relatively young, hot stars in this region. The edges of the galaxy appear less defined and fuzzier, indicating a decrease in stellar density and potentially an older stellar population. The overall shape is cigar-like, with no prominent spiral arms or other distinct features discernible. There is no obvious sign of ongoing major merger activity or significant tidal disruption. The galaxy shows minor disturbances.
