This galaxy presents as a single, relatively symmetrical object with a concentrated central region. There is a noticeable color gradient, shifting from a yellowish-white core to a bluer halo. The overall form appears smooth and somewhat diffuse, lacking a distinct spiral arm structure or strong morphological features. The absence of prominent dust lanes or tidal tails suggests that the galaxy is not currently undergoing a major merger event. The morphology is consistent with an early-type spiral or elliptical galaxy. Star formation is likely occurring, given the blue color of the halo, but is not a dominant process. There is some evidence of minor disturbances in the outer regions, potentially due to past interactions. Overall, this galaxy appears to be a fairly massive system with a moderate rate of star formation and a central core of older stars.
