The galaxy presents a generally smooth morphology, with a high degree of central concentration. The light is strongly concentrated, with a gradual falloff in intensity towards the outer regions. The shape is moderately elliptical, appearing nearly circular but slightly elongated. There is no clear evidence of spiral arm structure or a distinct disk. The color suggests an older stellar population, with a yellowish hue dominating the core. No signs of ongoing major mergers or significant tidal disturbances are visible. There is no discernible dust lane.
