The galaxy presents as a moderately bright, somewhat diffuse object with a generally smooth appearance, though not perfectly elliptical. There is a slight suggestion of a disk-like structure, though any spiral arms are not clearly defined or resolved within the image. The core appears brighter and more concentrated than the outer regions. Color gradients are present, with the inner regions seeming to exhibit a bluer hue, potentially indicative of younger stellar populations or ongoing star formation, while the outer regions tend toward redder tones, suggesting an older stellar population. There appears to be some disturbance in the structure. The galaxy exhibits a degree of asymmetry and possibly interaction with a smaller, nearby system.
