The galaxy presents as a lenticular or possibly an early-type spiral, seen at a shallow angle from our line of sight. A concentrated, bright bulge dominates the center, exhibiting a yellowish-orange hue, which indicates an older stellar population. A faint, flattened disk extends outwards from the bulge. The disk appears relatively smooth with little evidence of prominent spiral arm structure or large star-forming regions. The bluer colors observed at the disk's periphery suggest the presence of some younger stars, though not indicative of active, ongoing star formation at a high rate. There are no visible signs of any major mergers or significant tidal disturbances. The overall morphology suggests a system that may be transitioning from a more active, star-forming spiral to a passively evolving lenticular type.
