The galaxy appears to be a lenticular or early-type spiral galaxy, exhibiting a generally smooth, oval shape with minimal visible spiral arm structure. The central bulge is prominent and bright, showing a yellowish-white color indicative of an older stellar population. A fainter, bluer disk surrounds the bulge, suggesting some ongoing star formation, albeit at a relatively low rate. The galaxy shows a slight elongation, implying a possible disk structure viewed at an angle. There is no clear evidence of any major merger events or significant tidal disturbances in its vicinity. The overall morphology suggests a galaxy in a relatively quiescent state, transitioning from a more actively star-forming spiral to a more passive elliptical galaxy.
