The galaxy appears to be a relatively large, elliptical galaxy, exhibiting a smooth, symmetrical morphology. Its color profile suggests a population of older stars, indicated by its redder hue. There is little evidence of distinct spiral arms or significant dust lanes. The concentration of light is highest at the center, gradually diminishing outwards, fitting the profile of an elliptical galaxy. The absence of any distinct blue regions indicates a low rate of ongoing star formation. There is some slight asymmetry to the outer profile but overall the galaxy does not appear to be undergoing any major interactions or disturbances. The galaxy is moderately bright, suggesting a relatively high stellar mass. The general appearance points towards a quiescent, evolved system.
