This galaxy presents as a roughly elliptical form, appearing somewhat elongated in shape. The central region exhibits a bright, concentrated luminosity. The galaxy displays a smooth, rather than clumpy texture, suggesting a lack of significant ongoing star formation. A subtle color gradient is observed, with a bluer hue towards the outer edges. Evidence of a possible disturbance is noticed, perhaps a minor gravitational interaction which may indicate an ongoing or recent merger with another smaller galaxy, based on irregular morphological features. Although there may be a disk-like structure, its prominence is weak, and the galaxy overall appears to be bulge-dominated.
