The galaxy exhibits a prominent disk structure with evidence of spiral arms. The arms appear relatively well-defined, though slightly flocculent. There is a central bulge present, appearing moderately sized in relation to the overall galactic disk. The nucleus appears bright and concentrated, suggesting a high density of stars or potentially an active galactic nucleus. The overall color of the galaxy is skewed slightly towards the redder end of the spectrum, implying the presence of older stellar populations. Overall, the galaxy does not appear strongly disturbed, although minor disturbances can not be completely ruled out due to the image quality. There is a slight hint of a bar structure extending from the central bulge, but it appears weak or nascent. Star formation is likely occurring within the spiral arms, albeit at a relatively low rate. The galaxy's morphology suggests a type intermediate between a pure spiral and a lenticular galaxy, potentially undergoing a transition in its star formation activity.
