The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile is dominated by yellow and red hues, suggesting an older stellar population with minimal ongoing star formation. There's a subtle suggestion of a disk-like structure, but it's largely obscured by the dominant spheroid component. No significant spiral arm structure is discernible. There are no signs of major mergers or tidal disturbances. The galaxy appears relatively isolated and undisturbed.
