The galaxy presents as a moderately bright, elliptical-like structure with an apparent smooth morphology. There is a dominant central bulge that appears concentrated and relatively luminous. The main body of the galaxy shows a gradual decrease in surface brightness moving outward from the core. The galaxy exhibits a slight elongation, departing subtly from a perfectly circular shape. Faint hints of a disk-like feature may be present, but are not well-defined. There appears to be little or no evidence of ongoing, significant star formation within the galaxy, which is consistent with its overall smooth appearance. No signs of major mergers or tidal disturbances are readily apparent. Overall, the object appears to be a relatively evolved system.
