The galaxy presents a generally smooth, elliptical morphology. There is a concentrated central bulge, exhibiting a bright, yellowish-orange hue, suggesting a substantial population of older stars. The isophotes appear relatively regular and concentric, indicating a relaxed, dynamically stable structure. The light profile gradually fades towards the outer regions of the galaxy, showing a lack of distinct spiral arms or prominent star-forming regions. There is minimal evidence of tidal features or significant morphological disturbances, although a very slight asymmetry in the outer halo could potentially indicate a past minor interaction. The overall appearance suggests a relatively evolved system, likely a giant elliptical galaxy with a dominant population of older stars and a low rate of ongoing star formation.
