The galaxy presents as a relatively compact object with a generally elliptical morphology. It exhibits a smooth, centralized concentration of light, appearing nearly spherical with only a slight deviation from perfect roundness. There are no discernible spiral arms or bar features visible. The galaxy's core displays a bright, yellowish hue, suggesting a population of older stars. A faint, diffuse halo of bluer light surrounds the central region, possibly indicating the presence of a younger stellar population and ongoing, albeit subdued, star formation activity. No significant tidal distortions or signs of recent merger activity are apparent. The overall light distribution suggests a well-relaxed system, consistent with an early-type galaxy.
