The galaxy presents as an elliptical morphology, with a smooth, concentrated light distribution. The core exhibits a bright, yellowish hue indicative of an older stellar population. Proceeding outwards from the core, the light intensity gradually decreases into a less defined halo. No distinct spiral arms or prominent dust lanes are discernible. There is a slight elongation in the structure. The overall appearance suggests a system that is relatively relaxed and quiescent in terms of star formation activity. Minor disturbances or tidal features are not visually evident. The galaxy's morphology appears to be in a relatively late stage of evolution.
