The galaxy presents as a relatively smooth, elongated structure. Its central region appears more luminous and concentrated, exhibiting a yellowish-white hue, suggesting an older stellar population. Extending outward from the core, a fainter, less defined disk-like structure can be observed. The overall morphology leans toward a lenticular or early-type spiral galaxy, showing a bulge-dominated system with minimal apparent star formation. There is a subtle indication of a disk, however, with a slight blue tint. There is no obvious evidence of significant tidal disturbances or ongoing major mergers affecting the overall shape or appearance of the galaxy.