This galaxy appears to be a relatively smooth and concentrated elliptical or lenticular galaxy. It exhibits a centrally bright bulge that diminishes in surface brightness with increasing radius. The color profile shows a yellow or golden hue, suggesting a population of older stars and a reduced rate of ongoing star formation. There is little evidence of spiral arms or significant dust lanes. The overall morphology indicates a system that is likely well-evolved and dynamically relaxed. The galaxy appears to be moderately rounded in shape, trending more towards an elliptical form than a highly flattened disk. There is no clear indication of a major ongoing merger or significant tidal disturbances in its immediate vicinity.
