The galaxy presents a predominantly smooth morphology. The overall shape appears to be somewhere between round and elliptical, showing a slight elongation in one direction. There is a central, bright bulge region that is more concentrated, with the luminosity decreasing gradually outward. The color is largely consistent across the galaxy, tending towards the redder end of the spectrum suggesting an older stellar population. There is no distinct spiral structure visible, nor any indication of significant dust lanes or patchiness. There is no clear sign of any major ongoing merging activity or significant tidal disturbances, though some faint irregularities or minor disturbances cannot be ruled out based on the image resolution.
