This galaxy presents as a spiral type, characterized by a discernible disk structure with prominent spiral arms. The arms exhibit a somewhat open winding, tracing a path outwards from a central bulge region. The color distribution suggests active star formation within the spiral arms, indicated by bluish hues, while the bulge appears more yellowish, possibly indicating an older stellar population. The galaxy's disk is oriented at an angle to our line of sight. No strong bar feature is immediately apparent bisecting the bulge, though a subtle asymmetry hints at a possible weak bar structure. There is no obvious sign of major merger activity or significant tidal disturbances.