The galaxy presents a morphology consistent with a spiral or lenticular type. The central bulge appears prominent with a yellowish hue, indicative of an older stellar population. A faint disk is visible, oriented at an oblique angle to our line of sight, showing hints of spiral arm structure. The disk exhibits a bluer color, suggesting the presence of younger, hotter stars and ongoing star formation. The overall shape appears somewhat elongated. There is some visual evidence of minor disturbances or asymmetries in the disk, potentially indicating tidal interactions or past merger events. The galaxy appears relatively smooth with very little presence of dust lanes in the arms or bulge. 
