The galaxy presents as a relatively smooth, elliptical-like structure with a concentrated central bulge. The color profile indicates a yellowish core, potentially suggesting an older stellar population within the nucleus. A subtle blue hue is visible in the outer regions, possibly indicative of younger, hotter stars in areas where star formation may be occurring. The galaxy lacks any prominent spiral arm structures or other significant morphological features. There's no readily apparent evidence of an ongoing major merger event, although subtle irregularities might hint at minor disturbances. The overall round shape suggests that it is relatively relaxed dynamically.
