The galaxy presents as a relatively compact object, exhibiting a smooth, elliptical morphology. There is a dominant central bulge, indicating a concentration of older stellar populations. The galaxy appears to have a yellow-white hue, suggesting a lack of significant ongoing star formation. No prominent spiral arms or dust lanes are visible. There are no indications of any tidal disturbances, major mergers, or active galactic nuclei activity observable in this image. The light distribution of the galaxy appears mostly symmetrical, with an axial ratio indicating it is somewhere between round and cigar-shaped.
