The galaxy appears as a single, relatively smooth object. The light distribution suggests an elliptical morphology with a high degree of central concentration. There is little evidence of spiral arms or distinct features that would indicate a disk component. The galaxy exhibits a yellowish-white hue overall, which may suggest a population of older stars and relatively low levels of ongoing star formation. The galaxy does not appear to be undergoing a major merger or significant tidal interaction, but there may be evidence of minor disturbances in its light profile. The galaxy's overall roundness points to a system dominated by random stellar motions.
