The galaxy presents as a generally smooth and rounded structure, with a concentrated central bulge exhibiting a bright yellowish-white hue. The outer regions transition into a fainter, less defined halo with a slightly reddish tint. There's no clear indication of spiral arms or a defined disk component; rather, the light appears relatively uniform, suggesting an elliptical morphology. There is no obvious presence of significant dust lanes or active star-forming regions. The overall appearance is consistent with a relatively evolved galaxy, likely dominated by older stellar populations. There are no obvious signs of recent merger activity or major gravitational disturbances.
