The galaxy presents a generally smooth and rounded morphology. There appears to be a high degree of central concentration of light, characterized by a bright, yellowish core that suggests an older stellar population dominating the central region. The color gradient moving outward from the core does not indicate significant presence of young, blue stars. The light is relatively uniform with minimal signs of any distinct spiral arm structure or prominent dust lanes. There are no indications of ongoing major mergers or significant tidal disturbances. This galaxy exhibits features consistent with an elliptical galaxy.
