The galaxy presents an elongated, spindle-like morphology. The light distribution appears relatively smooth and centrally concentrated, with a bright core that fades gradually toward the outer regions. There's a hint of a disk-like structure. The color profile appears to be generally yellowish, suggesting a stellar population dominated by older stars. There is no strong evidence of active star formation regions within the galaxy based on the current data, indicating it is a relatively passive system. There is no clear indication of any major merger events, and no notable tidal features are visible.
