The galaxy appears as a generally smooth, elliptical-like structure. It exhibits a concentrated central bulge that is bright and yellowish in color, suggesting an older stellar population dominating the core. Fainter, diffuse extensions can be observed extending from the central region, though these lack distinct spiral arm features. There is a subtle color gradient, transitioning from the yellowish core to a somewhat bluer hue in the outer regions. This may indicate ongoing, though possibly subdued, star formation activity in these areas. No significant signs of major mergers or tidal disturbances are immediately apparent in this image.
