The galaxy presents as a relatively smooth, elliptical system. It exhibits a generally round morphology with a concentrated central bulge that appears slightly brighter than the surrounding regions. The color profile suggests an older stellar population, with a yellow-red hue dominating the galaxy's overall appearance. There is no clear evidence of significant dust lanes, spiral arms, or ongoing major mergers. Subtle irregularities in the outer regions may indicate minor tidal interactions or past accretion events, but the dominant impression is one of a relaxed, evolved galaxy. The galaxy's moderate size and luminosity suggest a substantial stellar mass. Overall, the morphological features are consistent with a galaxy that has largely completed its major star formation phase.
