The galaxy presents as a relatively smooth, elliptical-like structure. Its core exhibits a bright, concentrated luminosity, suggesting a high density of stars and possibly an active galactic nucleus, though this cannot be confirmed from the image alone. Moving outward from the core, the galaxy displays a gradual decline in brightness. There are hints of a disk but it is not a prominent feature. The overall color appears to be somewhat redder in the central regions, possibly indicating an older stellar population. Faint blue regions are visible and may indicate ongoing star formation, though the rate is not high. There is no obvious indication of a major merger event in the recent past; the galaxy shows little to no major disturbances.
