The observed galaxy presents a generally smooth morphology. The central region exhibits a concentrated brightness, appearing nearly circular in overall shape. There is a slight elongation apparent in the galactic structure. There may be a subtle indication of a very minor tidal disturbance or asymmetry in the outer regions, though this is difficult to determine given the resolution of the image. No clear spiral arm structures or distinct dust lanes are discernible. The galaxy appears to be isolated, showing no clear signs of ongoing major merger activity, however, there is a slight hint of a minor merger in the galaxy's outer regions. The galactic core presents a distinct color, potentially indicative of a unique stellar population or activity within the galactic nucleus.
