The observed galaxy presents as a centrally concentrated light source, appearing roughly circular in projection. The core exhibits a bright, compact morphology. The overall color appears slightly redder, with a smooth profile and no apparent spiral arm structure or prominent dust lanes. The light distribution decreases gradually with radial distance from the core, with no distinct features such as bars or rings visible at this resolution. The galaxy's appearance suggests a likely classification as an elliptical galaxy. However, the possibility of a smooth spiral galaxy viewed face-on cannot be ruled out without further spectroscopic data. There also appears to be some signs of disruption in the galaxy, that look like minor disturbances. These may be merger events that are currently ongoing.
