The galaxy presents an elongated, elliptical morphology. It exhibits a relatively smooth, diffuse light distribution, with no readily apparent spiral arm structures or strong dust lanes visible. The color gradient suggests a population of older stars, trending towards redder hues in the central region. The galaxy appears to be largely undisturbed, showing no signs of ongoing major mergers or strong tidal interactions. A slight asymmetry is possibly present in the outer isophotes, hinting at a minor disturbance, but this requires further investigation. Overall, the galaxy seems to be a relatively evolved system, likely an elliptical galaxy with a modest level of star formation. Its estimated size, at its redshift, makes it consistent with a typical galaxy of moderate mass.
