The galaxy presents an elliptical morphology, appearing elongated with a smooth, featureless structure. The light distribution suggests a central bulge that dominates the overall luminosity. Moving outwards from the core, the luminosity gradually decreases, forming a diffuse halo.

There's no distinct spiral arm structure visible, and any disk component is likely minimal. The color gradient is subtle, with the central region displaying a yellowish-white hue, possibly indicative of an older stellar population. The outer regions appear slightly bluer, suggesting the presence of younger stars, though to a lesser extent than observed in spiral galaxies.

There are no apparent signs of active galactic nuclei activity or significant dust lanes. The galaxy appears relatively undisturbed, with no obvious tidal tails or distortions suggesting recent merger events.
