The galaxy presents as a centrally concentrated, elliptical morphology. A smooth, diffuse light profile emanates from the core, gradually decreasing in intensity toward the outer regions. The central region exhibits a yellowish-white hue, potentially indicative of an older stellar population. A subtle reddish tint is observed in the more diffuse regions, suggesting the presence of a moderate amount of dust or a population of cooler, redder stars. There is no discernible spiral arm structure or significant evidence of recent major merger activity. The overall appearance suggests a relatively quiescent galaxy with ongoing, but low levels of star formation. The galaxy appears generally undisturbed.
