The galaxy presents as a relatively smooth, centralized light source with a generally elliptical morphology. It exhibits a concentrated core, gradually decreasing in luminosity towards its outer regions. Based on the coloration, there appears to be an old stellar population with a minimal presence of younger, bluer stars, suggesting a relatively low rate of on-going star formation. There is no apparent spiral arm structure or pronounced dust lanes visible in this image. The overall appearance points towards an evolved system, potentially an elliptical or lenticular galaxy, showing no clear signs of major disturbances or ongoing mergers.
