The galaxy presents a generally smooth appearance, exhibiting a central bulge that is slightly elongated. There is subtle evidence of a disk-like structure, although it is not strongly defined. The galaxy appears to be in a relatively undisturbed state, without any major signs of tidal interactions or ongoing mergers. Its color profile suggests a lack of significant active star formation. The overall morphology indicates that it is likely an intermediate-mass galaxy, transitioning between a spiral and elliptical form.
