The galaxy presents a generally elliptical morphology, displaying a prominent central bulge that appears bright and concentrated. The light distribution suggests a relatively smooth overall structure, with a noticeable lack of distinct spiral arms or other defined features. The galaxy exhibits a color gradient, transitioning from a yellowish-white hue in the core to slightly bluer tones in the outer regions. This color variation may indicate differential stellar populations or dust distribution. There's a suggestion of a faint disk, viewed at a high inclination, based on the elongated shape and what appears to be a thin band of bluer light traversing the galaxy's central region. No major disturbances or tidal features are immediately evident, implying that the galaxy is relatively undisturbed in its recent history.
