This galaxy exhibits a primarily smooth morphology. The overall form is elongated, presenting a notable cigar-shaped appearance. There are suggestions of internal structure, potentially a disk, however, the smoothness dominates its characteristics. We observe hints of disturbance with light that scatters away from the main body of the galaxy, but there are no clear tidal tails or bridges indicative of a major ongoing merger, or any significant signs of interactions. The color gradient indicates a higher concentration of older stellar populations or dust toward the central region, which appear to be less active.
