This galaxy presents as a primarily smooth, elliptical structure with a concentrated central bulge. The color profile shifts from a yellowish-white core to a redder periphery, indicative of an aging stellar population in the outer regions. There's a notable absence of prominent spiral arms or dust lanes, reinforcing the classification as an elliptical galaxy. The galaxy exhibits a generally round morphology with minimal deviations from sphericity. I observe no signs of ongoing major mergers or significant tidal disturbances that would disrupt its overall smooth and relaxed form, although there might be a minor asymmetry indicating a small interaction. Its apparent color suggests a population of older, redder stars and a relatively low rate of current star formation.
