The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a generally smooth and centrally concentrated morphology. The light profile is characterized by a bright central bulge that fades outwards. There is no evidence of strong spiral arm structure or dust lanes. The overall color is slightly redder, suggesting an older stellar population and lower star formation rate. The galaxy has a moderate elliptical shape, and does not appear to be undergoing any major merging activity or significant tidal disturbance, but perhaps a slight distortion. The size is moderate.
