The galaxy presents a generally smooth morphology, with a noticeable absence of prominent spiral arms or distinct star-forming regions. The light distribution is concentrated towards the central region, suggesting a well-defined galactic nucleus. The overall shape of the galaxy appears elliptical, elongated along one axis, and exhibits a gradual decrease in luminosity from the core outwards. The color profile is predominantly yellow and red, indicating an older stellar population, though bluer tints can be observed in the very outer regions of the galaxy, indicating the presence of some younger stars there. There is no obvious indication of ongoing major merger activity, though minor tidal disturbance cannot be ruled out. The galaxy's structure suggests it is likely an elliptical galaxy.
