The galaxy presents as a smooth, elliptical-like object. Its core region exhibits a relatively high surface brightness, gradually diminishing towards the outer edges. The galaxy is generally round with some elongation visible. No distinct spiral arms or prominent dust lanes are apparent. There is no obvious evidence of recent or ongoing major merger activity or significant tidal disturbances. Color gradients suggest a stellar population that is slightly redder in the central regions compared to the outer parts. There are no particularly bright or well-defined star-forming regions visible, indicating a relatively low star formation rate. The galaxy's morphology suggests it is a relatively massive system with an evolved stellar population.
