The galaxy appears as a relatively smooth, centrally concentrated object with a slightly elliptical shape. There is a subtle color gradient, with the core region exhibiting a slightly warmer tone compared to the outer regions. While not distinctly spiral, there are faint hints of disk-like structure within the galaxy's overall form. There is no clear indication of active star formation regions or prominent dust lanes visible. The overall appearance suggests a relatively evolved galaxy, potentially an early-type spiral or a lenticular galaxy. It appears to be relatively isolated, without any obvious signs of major interaction or merging with nearby galaxies, although there may be a minor disturbance in its morphology. The galaxy's estimated size places it within a typical range for galaxies at its distance.
