The galaxy presents as a relatively smooth, elliptical-like structure. It exhibits a concentrated central bulge region that appears yellowish, suggesting an older stellar population. There is a subtle gradient in color and brightness, with the core being the most luminous. Surrounding the bulge is a more diffuse halo, which transitions to a bluer hue. This may indicate the presence of younger stars in this area, or perhaps it is simply a manifestation of the diminishing intensity of the yellowish light from the core. 

The overall shape is somewhat elongated, but it is difficult to assess the precise axial ratio given the image quality and the viewing angle. I detect minimal signs of active star formation; it appears to be a largely quiescent system. There is no evidence of strong spiral arm structures or significant dust lanes. I do detect a small object to the left of the galaxy. Although it is hard to tell at this resolution, it could be a dwarf galaxy in the process of merging. There does not appear to be strong signs of tidal distortions or interactions.
