The galaxy appears to be an elliptical galaxy, exhibiting a largely smooth and centrally concentrated morphology. It presents a somewhat elongated shape, leaning more towards an "in-between" roundness. The light profile suggests a relatively homogenous stellar population across the galaxy, with a gradual decrease in intensity from the core outwards. The core itself appears to be yellowish-white in color. There is no obvious evidence of spiral arms, a bar structure, or significant dust lanes. No apparent signs of ongoing major merger activity or significant tidal disturbances are observed. A very slight bluing is noted in the outer regions.
