This galaxy presents as a highly elongated, cigar-shaped structure. The light distribution appears relatively smooth, lacking prominent spiral arms or distinct features. The central region exhibits a concentration of yellowish light, suggesting an older stellar population. Fainter, bluer light extends outwards from the core, possibly indicating some ongoing star formation. There is no clear evidence of major mergers or significant tidal disturbances, suggesting a relatively isolated evolution. The galaxy appears to be a disk galaxy seen edge-on, with its light distributed across roughly 6 kpc.
