The galaxy presents as a moderately inclined, disk-like system. Its morphology appears smooth, with a notable lack of distinct spiral arm structure. A central bulge is evident, exhibiting a yellowish hue, which may indicate an older stellar population. The outer regions of the disk display a bluer color, potentially signifying ongoing star formation. The elongated shape suggests a classification leaning towards an edge-on spiral or lenticular galaxy. The disk appears relatively undisturbed, showing no obvious signs of major mergers or tidal interactions. There might be some minor irregular features that indicate minor disturbances from a small close-by object. Further spectroscopic analysis would be necessary to confirm the galaxy's redshift, stellar population characteristics, and star formation rate to better understand its composition and evolutionary history.
