The galaxy presents a largely smooth, elliptical morphology. Its core appears as a bright, concentrated central bulge, exhibiting a yellow-orange hue. The light intensity gradually decreases outwards from the core. The overall shape is generally round, although there may be a slight deviation from perfect circularity. There is no visual evidence of significant spiral arm structure or strong tidal disturbances, but the overall diffuse glow may obscure minor disturbances if present. The galaxy seems to have a generally old stellar population, as indicated by the yellow-orange colour, suggesting a lack of ongoing star formation within the observed spectral range.
