The galaxy presents as an elliptical morphology, elongated significantly along its major axis. The central region exhibits a higher surface brightness, indicative of a concentrated stellar population, likely an older population dominating the core. Progressing outward from the core, the luminosity gradually decreases with no distinct features such as spiral arms or a prominent disk visible. The color profile demonstrates a redder hue overall, suggesting a lack of significant recent star formation throughout the galaxy. The high concentration and lack of blue colors associated with active star formation suggest that this galaxy is likely a quiescent elliptical galaxy with a spheroidal shape and a dominant old stellar population.
