The galaxy presents as a spiral type, exhibiting a prominent disk structure. The spiral arms are clearly defined, demonstrating a morphology characterized by a two-armed structure. The winding of the spiral arms appears to be of medium tightness. A central bulge is discernible, of moderate size relative to the disk. Evidence suggests the presence of a strong bar feature bisecting the central bulge and extending into the inner disk. The galaxy shows a slight inclination relative to our line of sight, allowing for partial visualization of the disk structure. There are indications of minor disturbances, and potentially interactions with smaller companions. Color gradients are visible, with the central regions displaying yellowish hues, potentially indicative of an older stellar population, while the spiral arms exhibit bluer tones, potentially indicating ongoing star formation.
