The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a smooth, relatively featureless morphology. It displays a central bulge that appears moderately bright and concentrated, with a yellowish hue indicating an older stellar population. A faint disk is visible, though its structure is not clearly defined, showing a slight elongation. There is little evidence of active star formation within the disk, as indicated by the lack of prominent blue regions or HII regions. Overall, the galaxy seems to be a relatively evolved system with a dominant spheroidal component and a subdued disk. Weak disturbance in structure present suggesting minor interaction with nearby galaxies. 
