This galaxy presents a generally smooth, elliptical morphology. A bright central bulge dominates the structure, exhibiting a concentrated luminosity profile. There is a disk-like feature, but it appears relatively faint and unresolved, with a low surface brightness compared to the bulge. A slight disturbance is present at one edge. There are no distinct spiral arms or strong bar structures visible. Color gradients across the galaxy suggest variations in stellar populations or dust content. The galaxy appears relatively isolated, with no obvious signs of major merging activity.
