The galaxy appears to be an elliptical galaxy, exhibiting a generally smooth and featureless morphology. It presents an elongated shape with a noticeable central bulge, suggesting a concentration of older stellar populations. The color gradient shifts from a slightly yellower hue in the core to a bluer tint in the outer regions. The bluer tones possibly indicates a degree of ongoing, albeit relatively low-level, star formation towards the outskirts. There is no definitive indication of active galactic nuclei. Weakly defined boundaries do not indicate a strong interaction with other galaxies, though a minor disturbance cannot be excluded at this resolution.
