The galaxy appears as a concentrated spheroid with a smooth light distribution, suggesting an elliptical morphology. The light profile is centrally concentrated with a gradual decline in intensity outward, indicating an older stellar population lacking significant ongoing star formation. There is no evidence of spiral arms or a prominent disk structure. The galaxy exhibits a moderate redshift, placing it at a significant cosmological distance. The color indices indicate a redder overall color, consistent with an evolved stellar population dominated by older stars. There are no obvious signs of recent major merger activity, such as tidal tails or strong asymmetries. It is relatively isolated in this field, indicating a low-density environment.
