The galaxy presents a generally smooth, elliptical morphology. The central region exhibits a bright, concentrated luminosity, indicative of a significant stellar population and potentially a supermassive black hole at its core. There is little evidence of significant star formation occurring. Its shape is generally oval, exhibiting more rounded characteristics. There's no readily apparent evidence of a recent or ongoing major merger event, though some minor irregularities in the outer regions suggest a possibility of smaller past interactions. 
