The galaxy presents an elliptical morphology, appearing as a diffuse spheroid with a relatively smooth light distribution. There is an indication of a central concentration of light, suggesting the presence of a galactic nucleus. A slight elongation is observed, though no distinct spiral arm structures or features of active star formation are apparent. The color gradient suggests a population of older stars, with a possible subtle central disk that could be comprised of somewhat younger and bluer stars. There is no evidence of any on-going major merger activity.