The galaxy presents as a lenticular or edge-on spiral. It displays a relatively smooth, centrally concentrated bulge, exhibiting a soft blue-white hue. The disk component appears elongated with a diffuse glow, lacking distinct spiral arm structure. The overall color is subtly blue-shifted, suggesting a moderate population of young, hot stars within the disk, though the star formation rate appears relatively low. The morphology suggests a galaxy that is either evolving from a spiral to an elliptical or a gas-poor spiral with a suppressed star formation rate. The galaxy appears undisturbed, with no signs of ongoing major mergers. A slight asymmetry in the outer regions may indicate a minor gravitational interaction or past accretion event. The redder color at the central bulge region suggests an older stellar population compared to the disk. The shape is cigar-like when viewed from this angle.
