The galaxy presents as a spiral type, exhibiting a distinct central bulge that appears moderately sized. Faint spiral arm structures are visible, though not sharply defined. The galaxy's disk is not viewed edge-on, presenting at an angle that allows some clear view of spiral structure. There appears to be no strong bar structure present. There may be some distortion or minor disturbance suggesting possible past or ongoing interaction with another galaxy, but overall the morphology is fairly relaxed. The central bulge exhibits a yellow-red hue, suggesting an older stellar population. The spiral arms exhibit a bluer tinge, indicating the presence of younger, hotter stars and ongoing star formation.
