The galaxy appears as a centrally concentrated object, exhibiting a smooth, elliptical morphology. It is slightly elongated with a subtle cigar shape. There is no apparent spiral structure or obvious disk. The color profile suggests a population of older stars, indicated by the reddish-yellow hue in the central region. There is a faint blue color in the edges of the galaxy, suggesting the presence of some younger, hotter stars. There are no signs of major disturbances or merging events in the system.
