The galaxy presents as a centrally concentrated, luminous object, likely a lenticular or early-type spiral galaxy at an estimated distance correlating to a redshift of approximately z = 0.17. The morphology appears largely smooth, with a high degree of central bulge dominance. There is very little evidence of spiral arm structure or prominent star-forming regions within the galaxy. The light is dominated by redder wavelengths in the core, suggesting an older stellar population and reduced current star formation. The outer regions of the galaxy exhibit a faint disk-like structure, presenting a bluer hue, potentially indicating the presence of a small population of younger stars within the extended galactic plane. There is no noticeable sign of strong tidal interactions or significant morphological disturbances, which implies the galaxy has likely experienced a relatively quiescent evolutionary history. It appears to be an isolated system with no merging or tidal features. 
