The galaxy presents as a relatively compact structure, appearing generally smooth in overall texture, but not perfectly spherical. The light distribution appears concentrated towards the center, with a gradual decline in intensity towards the outer regions of the galaxy.

There may be subtle signs of disturbances or features, such as a hint of asymmetry or faint, diffuse extensions, potentially indicating past minor interactions or internal processes. I observe a hint of disk-like structure, but it seems relatively face-on. There is no distinct dust lane visible. Based on its color, it appears to be composed of both older stellar populations. Blue regions of the galaxy suggest a population of young, hot stars, indicating ongoing star formation.
