The galaxy presents a smooth, elliptical morphology. It appears elongated, exhibiting a cigar-like shape. The central region displays a bright, concentrated luminosity, suggesting a high stellar density. The light profile gradually fades towards the outer edges, exhibiting no apparent spiral arm structures or prominent dust lanes. There is no indication of active galactic nuclei activity or intense star formation occurring within the observable wavelengths. Minor disturbance is possible, but not readily apparent. The galaxy exhibits a colour gradient, with the core appearing slightly yellow compared to the redder outer regions.
