The galaxy appears to be elliptical in morphology, exhibiting a predominantly smooth light distribution. It has a notable central concentration of light, appearing almost spherical, with the isophotes becoming less dense toward the outer regions. The galaxy displays a yellow-red hue centrally, indicative of an older stellar population. Fainter, more diffuse blue regions surround the central core. There appear to be some minor disturbances in the outer regions, suggesting possible past interactions. There may be some evidence of disk structure; it would be hard to say for certain without a better image.