The galaxy presents a somewhat elongated, cigar-shaped morphology. It appears relatively smooth in structure, with a notable absence of well-defined spiral arms or prominent dust lanes. The color profile suggests a central bulge that is more yellow/red, indicative of an older stellar population and potentially significant dust obscuration, while the outer regions exhibit a bluer hue, suggesting the presence of younger, hotter stars and ongoing star formation. The galaxy doesn't show any signs of major mergers or strong tidal disturbances.
