The galaxy presents a generally elliptical morphology with a smooth, diffuse structure, lacking prominent spiral arms or a well-defined disk. The central region exhibits a bright, concentrated core that decreases in luminosity moving outwards. The galaxy's color profile indicates a redder hue, suggesting a population of older stars and a lower rate of ongoing star formation, which correlates with an older stellar population. There are no readily apparent signs of active galactic nuclei activity or dust lanes within the image's resolution, but some disturbance is visible in the outer regions which may be due to recent mergers or interactions. 
