The galaxy presents an elongated, cigar-shaped morphology. Its light profile appears relatively smooth and centrally concentrated, lacking any obvious spiral arm structure or distinct knots of star formation. The color gradient suggests a redder core, with a gradual shift towards bluer hues at the periphery. The overall appearance suggests a mature stellar population, potentially an elliptical or lenticular galaxy viewed nearly edge-on. There appears to be no significant signs of recent mergers or tidal disturbances affecting the system. The smoothness of the galaxy indicates it is likely stabilized, and any recent star formation rates are low.
