The galaxy appears to be of elliptical morphology, displaying a generally smooth light distribution with no readily apparent spiral arms or distinct features. The light is concentrated in a bright, relatively compact core region. Moving outwards from the core, the light intensity decreases gradually into an extended halo. Subtle color gradients may be present, with the inner regions appearing more yellow or red, suggesting an older stellar population compared to bluer tints in the outskirts. There might be subtle indications of tidal disturbances or faint streams suggesting a past interaction or minor merger event, though these features are not prominent. The overall structure indicates a evolved system with potential for a complex dynamical history.
