The galaxy presents as a cigar-shaped, elongated structure with a significant degree of internal smoothness. The light distribution suggests a central bulge, although distinct spiral arm features are not readily discernible. The galaxy exhibits a color gradient, transitioning from a slightly bluer hue at the outer edges, indicative of younger stellar populations and ongoing star formation, to a redder core, suggesting an older, more evolved stellar population. The galaxy doesn't appear to be undergoing any major merging events, although there is a possibility for minor disturbances.
