The galaxy appears as a relatively smooth, centrally concentrated object. There is a bright, compact core that suggests a possible bulge component. The galaxy presents an overall elliptical morphology with a high degree of roundness, showing only a small deviation from a perfect circular shape. The color profile suggests the presence of a moderately old stellar population, as indicated by the subtle reddish hues. Faint, diffuse light extends outwards from the core, without evidence of spiral arm structures or significant dust lanes. There is a hint of disturbance or faint tidal features in the outer regions.
