The galaxy appears as a centrally concentrated object, exhibiting a smooth and somewhat rounded morphology. A prominent central bulge dominates the visual structure, characterized by a yellowish-orange hue, suggesting an older stellar population. Fainter, bluer diffuse light extends outwards from the core region, likely indicating the presence of a younger stellar population. There is no apparent spiral arm structure or significant dust lanes visible in this image. There appears to be little if any significant disturbance or tidal features, implying relative isolation and gravitational stability. The color profile suggests ongoing, albeit low, levels of star formation.
