The galaxy presents as a relatively smooth, elliptical morphology. It exhibits a concentrated central bulge with a gradual fading in luminosity outwards. The overall shape appears largely spheroidal, with a high degree of roundness, though there is a suggestion of a slight extension along one axis. The color gradient suggests a population of older stars dominating the core, indicated by the yellow hue. There are no clear spiral arms or distinct dust lanes visible. Faint traces of bluer light at the edges of the galaxy could indicate some ongoing, albeit weak, star formation in the outer regions. There's a hint of possible tidal disturbance present, though the image resolution makes it challenging to confirm with certainty, perhaps suggestive of a past or ongoing minor interaction. The distribution of light appears largely symmetrical, with no obvious signs of a recent major merger.
