The galaxy appears to be elliptical in shape, exhibiting a smooth, diffuse light profile. The core region is significantly brighter, suggesting a high concentration of stars and possibly a supermassive black hole at its center. The overall color of the galaxy leans towards the redder end of the spectrum, indicative of an older stellar population with reduced star formation activity. There is a hint of possible tidal disturbance in the form of a very faint extension, although the image quality limits conclusive determination. This feature could also be due to image artifacts, as the main body of the galaxy otherwise shows no strong signs of ongoing interaction or merging events.
