The galaxy presents a largely smooth, elliptical appearance with a central, luminous bulge. There is evidence of a surrounding disk. The color gradient suggests the presence of varying stellar populations; the central region exhibiting a yellow-orange hue, indicative of older, evolved stars, while the outer disk displays a bluer tint, suggesting the presence of younger, hotter stars and active star formation. The galaxy does not appear to be undergoing any major mergers, however there are some minor disturbances that can be seen. It maintains a relatively circular form.
