The galaxy presents a largely smooth, elliptical morphology with an apparent lack of distinct spiral arms or a bar structure. The central region exhibits a high surface brightness, indicative of a dense stellar population or possibly an active galactic nucleus, though further spectroscopic data would be necessary to confirm this hypothesis.

The overall shape is somewhat elongated, with a discernible deviation from perfect sphericity; it is more "in between" than "round" in shape. There is some evidence of faint outer regions of diffuse light extending away from the core, suggesting a possible extended stellar halo. The galaxy appears to be relatively isolated with no obvious signs of ongoing major merger activity, though a minor disturbance cannot be ruled out based on the data available. Color gradients are subtle, with a generally redder hue, indicative of an older stellar population and comparatively low ongoing star formation.
