The galaxy presents as a lenticular or early-type spiral galaxy, seen at a slight oblique angle. It exhibits a prominent bulge, which appears smooth and centrally concentrated with a yellowish hue. The disk component is subtly visible, displaying a fainter and bluer color compared to the bulge. There appears to be a very slight hint of spiral arm structure in the disk, but it's difficult to definitively confirm. The overall morphology suggests a relatively evolved system, with a dominant old stellar population. There is no significant evidence of ongoing major star formation within the galaxy, and no obvious signs of tidal disturbances or merging events.
