The galaxy presents as a relatively compact and moderately luminous system at a redshift of approximately 0.039. Its morphology appears to be that of a spiral galaxy with a degree of internal disruption. The central region exhibits a concentration of older stellar populations, indicated by its yellowish-white color. Surrounding this central bulge, fainter spiral arm segments can be discerned. These arms are bluer in color, suggesting the presence of ongoing star formation within them. Patches of redder regions are sparsely distributed in the outer regions, possibly indicative of dust. The overall light profile suggests a relatively low star formation rate compared to the galaxy's inferred mass. There's a possible indication of a minor interaction, showing hints of tidal features or slight morphological disturbances in the outer halo of the galaxy.
