The galaxy presents a largely smooth and centrally concentrated morphology, appearing elliptical in shape. Its light profile is characterized by a diffuse glow that gradually fades outward from a bright core. A slight elongation is discernible, but it is generally round in appearance. There is no evidence of spiral arms, a bar structure, or significant dust lanes. The color appears to be a blend of red and blue, with a bias toward redder hues, which suggests an older stellar population. There are no obvious signs of ongoing major mergers or significant tidal disturbances, although a faint, irregular structure can be observed, potentially indicating a minor disturbance or interaction. There is no evidence of strong star formation based on the color and lack of bright, blue knots usually associated with active star-forming regions.
