The galaxy presents a morphology characterized by both smooth and featured components. The overall form appears somewhat elliptical, though not perfectly so. The central region is noticeably brighter and more concentrated, with a yellowish-orange hue, suggesting an older stellar population. Fainter, diffuse bluish patches are visible in the surrounding area, potentially indicating regions of more recent star formation.

There is evidence of gravitational disturbance in the morphology; specifically, a second, smaller, and more diffuse object appears closely associated, potentially either a smaller galaxy undergoing a merger or tidal debris from a previous interaction. The main body of the galaxy seems to be exhibiting slight distortions or irregularities, further hinting at an ongoing or recent interaction. Redder regions can be observed, potentially due to dust and reddened light from background stars.
