The galaxy presents as a relatively compact object with a notable central bulge. The morphology appears to be largely smooth, with only subtle indications of spiral arm structure or features beyond a general disk shape. The galaxy exhibits a color gradient, transitioning from a yellowish-white core region outward to a bluer halo. Some asymmetry is present in the outer halo, potentially suggesting some tidal interaction or past merger event, although the overall structure is not significantly disturbed. Based on the red color of the center, we can infer that the core of the galaxy hosts old stars and little ongoing star formation. The relatively blue color of the halo suggest some degree of star formation occurring in this outer region. Overall, the galaxy exhibits characteristics of a possible lenticular or early-type spiral galaxy at an intermediate distance.
