The galaxy appears to be a relatively compact system, presenting a generally smooth morphology. There is a hint of a disk-like structure, although the overall appearance is dominated by a more spheroid, elliptical-like profile. The central region is noticeably brighter, exhibiting a yellowish hue. This may indicate an older stellar population concentrated towards the core. Moving outward, there is a slight gradient towards bluer colors at the edges, which could imply the presence of younger, hotter stars in the outer regions. Overall, the galaxy shows minimal signs of significant disturbance or recent major mergers. There is a subtle asymmetry, which could be a sign of a minor interaction or internal dynamical process.
