This galaxy exhibits a relatively smooth morphology, with a dominant central bulge that appears quite luminous. The galaxy's color suggests an older stellar population, particularly within the central bulge, with a yellow-red hue. There is some evidence of a fainter, disk-like structure extending from the central region, but it is not well-defined. The asymmetry in the light distribution implies possible tidal interactions or minor disturbances. A faint, elongated feature, potentially a tidal tail, is visible near the galaxy. Overall, this appears to be a relatively massive galaxy at moderate redshift, with a dominant bulge and signs of past or ongoing interactions.
