The galaxy presents as a lenticular or possibly early-type spiral galaxy, oriented nearly edge-on to our line of sight. The central bulge appears bright and concentrated, exhibiting a yellowish hue suggestive of an older stellar population. A faint, flattened disk is visible, extending outwards from the bulge along the horizontal axis, with hints of blueish concentrations that could indicate regions of active star formation. While predominantly smooth, the galaxy shows minor asymmetries in its outer regions, possibly indicating a minor gravitational interaction or internal disturbances. The overall morphology is that of a relatively massive galaxy with moderate star formation, though the limited resolution obscures any detailed structural features within the disk.
