This galaxy presents as a centrally concentrated object with a smooth, elliptical morphology. The light profile appears to gradually decrease in intensity from the core outwards. There is a slight reddish hue, indicating a potentially older stellar population and/or significant dust content, primarily in the core. No distinct spiral arm structures or prominent star-forming regions are discernible. The galaxy appears generally undisturbed with no evidence of tidal tails, bridges, or other significant morphological distortions, although there could be very weak disturbances. The overall shape is very round and the galaxy appears to be in a relatively relaxed state.
