The subject galaxy presents as an elongated, spindle-shaped structure. Its color profile suggests the presence of an older stellar population, with a concentration of light towards the redder end of the spectrum. The morphology appears to be that of a disk galaxy viewed nearly edge-on. There is no discernible bulge component. No active star-forming regions are obviously visible. The galaxy appears relatively undisturbed, showing no strong signs of recent or ongoing mergers or tidal interactions.
