The galaxy presents as a relatively compact, rounded structure. Its light profile appears generally smooth, without prominent spiral arms or a distinct bar. There's a subtle central concentration of light, suggesting a bulge component. The galaxy's overall color is moderately red, indicating a stellar population that is relatively old, or obscured by dust. There's no strong evidence of recent or ongoing major mergers, although minor disturbances are possible, and cannot be ruled out given the image resolution. The lack of intense blue regions implies a low star formation rate.
