The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a smooth, elliptical morphology with a prominent bulge. The light is dominated by older stellar populations, inferred from the yellowish-orange color towards the center. There's a subtle blueish tint along the outer edges which may indicate some recent star formation, but overall the galaxy lacks prominent spiral arm structures. The disk appears relatively smooth and featureless, with no distinct dust lanes or HII regions easily visible. The overall shape is elongated, suggesting an elliptical profile rather than a perfectly circular one. There is little evidence of a major ongoing merger, though some slight asymmetry in the outer regions could suggest minor tidal interactions or past accretion events. The galaxy appears relatively isolated, with no close companions visibly interacting with it.
