The galaxy presents as a somewhat elongated object, with a notable central bulge. The core region is a concentrated area of light, appearing yellowish-orange in color, indicating an older stellar population and lower levels of ongoing star formation within the nucleus. Surrounding the central bulge, fainter and bluer regions are visible, particularly at the extremities of the galaxy's major axis. These suggest areas of more recent star formation and the presence of younger, hotter stars. The overall structure appears relatively undisturbed, exhibiting only minor asymmetries and a relatively smooth appearance. There are hints of a disk-like structure, but the high degree of inclination complicates a confident classification. The morphological assessment indicates it may be an early-type spiral galaxy, viewed at an angle, or potentially a lenticular galaxy. The spiral arms, if present, are not clearly defined.
