The galaxy presents a generally smooth, elliptical morphology with a slightly elongated shape. The central region exhibits a concentrated, bright core, suggesting a significant stellar population and potentially a supermassive black hole. A faint, diffuse halo extends outwards from the core, gradually fading into the background. There is some visual indication of asymmetry and a potential disturbance in the galaxy's outer regions, possibly indicating tidal interactions or a minor merger event. The galaxy appears to be dominated by older stellar populations, as indicated by the reddish-yellow hue of the central region, although a hint of bluer light suggests the presence of some younger stars in the outer regions.
