The galaxy presents as a relatively smooth, elliptical-like structure with a dominant, concentrated central bulge. There's a general absence of prominent spiral arms or distinct morphological features suggestive of ongoing mergers or major disturbances. The galaxy appears moderately rounded, displaying a shape more akin to a sphere than a flattened disk when observed from our vantage point. There is minimal evidence of significant dust lanes or active star-forming regions contributing to the overall color profile.
