The galaxy presents a morphology consistent with a lenticular or early-type spiral. It exhibits a prominent bulge, which is yellowish-white in color, suggesting an older stellar population with minimal ongoing star formation within that region. A faint disk component is visible, extending outwards from the bulge. The disk displays a bluer hue than the bulge indicating younger stars and some star-forming regions. The overall shape is flattened, with an elliptical appearance but not extremely so. No obvious spiral arms are immediately apparent, potentially indicating tightly wound arms or a relatively smooth disk structure. There might be minor tidal disturbance or some minor interaction present, as there is a slight asymmetry noticeable in the disk's outer regions. This galaxy likely represents a system that is transitioning from a spiral to a lenticular type morphology.
