The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a smooth, centrally concentrated bulge. The disk component is present, but its features are not well-defined, possibly due to the viewing angle, which seems close to edge-on. The color profile suggests older stellar populations, concentrated towards the center, with relatively less active star formation. The overall morphology hints at a relatively massive system that may be transitioning from a spiral to an elliptical type, or has already done so. There is no obvious tidal disruption of nearby galaxies, although a minor interaction cannot be fully ruled out based solely on this image.
