The galaxy appears to be a lenticular galaxy, characterized by a smooth, relatively featureless disk. The galaxy exhibits a notable bulge component, evidenced by the concentrated light in the central region. The color of the bulge appears slightly redder than the disk, which could suggest an older stellar population. There is little evidence of spiral arm structure or prominent dust lanes within the disk, suggesting the galaxy is relatively quiescent in terms of star formation. The overall morphology is smooth and rounded, with a slight elongation indicative of a disk viewed at an intermediate inclination angle. There are no strong signs of recent merger activity or major disturbances. The galaxy has a relatively compact structure, its light is concentrated within a small area.
