The galaxy presents as a roughly elliptical structure, exhibiting a smooth, concentrated central bulge. The bulge appears yellowish, suggesting an older stellar population. A faint, bluish disk surrounds the bulge, implying the presence of some younger, bluer stars and possibly ongoing star formation. There appears to be some minor disturbances visible in the outer regions of the disk, which could indicate the presence of a minor merger event or interaction with another galaxy in its past. The galaxy exhibits a moderate degree of roundness, appearing neither perfectly spherical nor highly elongated. Overall, it appears to be a galaxy undergoing a relatively quiet period of evolution.
