The galaxy appears to be a relatively smooth, elliptical galaxy. It exhibits a concentrated central bulge and a fainter, diffuse halo surrounding it. The galaxy appears to be moderately flattened, with an aspect ratio that suggests it is not perfectly spherical, but rather somewhat elongated. There is a subtle color gradient, transitioning from a slightly bluer hue in the central region to a redder, more muted color in the outer regions. The overall light distribution is smooth and lacks any prominent spiral arms or distinct features. There are no clear signs of ongoing major mergers or significant tidal disturbances. The galaxy's morphology suggests that star formation is likely suppressed, with an older stellar population dominating the overall light emitted.
