The galaxy presents as a relatively compact object with a smooth, diffuse light distribution. There is a slight elongation, appearing somewhere between round and cigar-shaped, but it is predominantly elliptical in form. A distinct color gradient is observed, transitioning from a yellowish central region to bluer outer edges. This suggests variations in stellar populations, with potentially older, redder stars concentrated towards the core and younger, bluer stars residing in the outskirts. No prominent spiral arms or bar structures are visible, and the galaxy's overall structure appears largely undisturbed. There is a region of blue light to the left of the main galactic body, which could be a region of star formation within the galaxy or a separate galaxy that may be merging. The galaxy exhibits a moderate redshift, indicating it is at a considerable distance.
